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The remnants of galaxy formation from a panoramic survey of the region around M31

Identifieur interne : 003429 ( PascalFrancis/Curation ); précédent : 003428; suivant : 003430

The remnants of galaxy formation from a panoramic survey of the region around M31

Auteurs : Alan W. Mcconnachie [Canada] ; Michael J. Irwin [Royaume-Uni] ; Rodrigo A. Ibata [France] ; John Dubinski [Canada] ; Lawrence M. Widrow [Canada] ; Nicolas F. Martin [Allemagne] ; Patrick Cote [Canada] ; Aaron L. Dotter [Canada] ; Julio F. Navarro [Canada] ; Annette M. N. Ferguson [Royaume-Uni] ; Thomas H. Puzia [Canada] ; Geraint F. Lewis [Australie] ; Arif Babu [Canada] ; Pauline Barmby [Canada] ; Olivier Bienayme [France] ; Scott C. Chapman [Royaume-Uni] ; Robert Cockcroft [Canada] ; Michellel M. Collins [Royaume-Uni] ; Mark A. Fardal [États-Unis] ; William E. Harris [Canada] ; Avon Huxor [Royaume-Uni] ; A. Dougal Mackey [Royaume-Uni] ; Jorge Penarrubia [Royaume-Uni] ; R. Michael Rich [États-Unis] ; Harvey B. Richer [Canada] ; Arnaud Siebert [France] ; Nial Tanvir [Royaume-Uni] ; David Valls-Gabaud [France] ; Kimberly A. Venn [Canada]

Source :

RBID : Pascal:09-0386067

Descripteurs français

English descriptors

Abstract

In hierarchical cosmological models', galaxies grow in mass through the continual accretion of smaller ones. The tidal disruption of these systems is expected to result in loosely bound stars surrounding the galaxy, at distances that reach 10-100 times the radius of the central disk2,3. The number, luminosity and morphology of the relics of this process provide significant clues to galaxy formation history4, but obtaining a comprehensive survey of these components is difficult because of their intrinsic faintness and vast extent. Here we report a panoramic survey of the Andromeda galaxy (M31). We detect stars and coherent structures that are almost certainly remnants of dwarf galaxies destroyed by the tidal field of M31. An improved census of their surviving counterparts implies that three-quarters of M31's satellites brighter than Mv = -6 await discovery. The brightest companion, Triangulum (M33), is surrounded by a stellar structure that provides persuasive evidence for a recent encounter with M31. This panorama of galaxy structure directly confirms the basic tenets of the hierarchical galaxy formation model and reveals the shared history of M31 and M33 in the unceasing build-up of galaxies.
pA  
A01 01  1    @0 0028-0836
A02 01      @0 NATUAS
A03   1    @0 Nature : (Lond.)
A05       @2 461
A06       @2 7260
A08 01  1  ENG  @1 The remnants of galaxy formation from a panoramic survey of the region around M31
A11 01  1    @1 MCCONNACHIE (Alan W.)
A11 02  1    @1 IRWIN (Michael J.)
A11 03  1    @1 IBATA (Rodrigo A.)
A11 04  1    @1 DUBINSKI (John)
A11 05  1    @1 WIDROW (Lawrence M.)
A11 06  1    @1 MARTIN (Nicolas F.)
A11 07  1    @1 COTE (Patrick)
A11 08  1    @1 DOTTER (Aaron L.)
A11 09  1    @1 NAVARRO (Julio F.)
A11 10  1    @1 FERGUSON (Annette M. N.)
A11 11  1    @1 PUZIA (Thomas H.)
A11 12  1    @1 LEWIS (Geraint F.)
A11 13  1    @1 BABU (Arif)
A11 14  1    @1 BARMBY (Pauline)
A11 15  1    @1 BIENAYME (Olivier)
A11 16  1    @1 CHAPMAN (Scott C.)
A11 17  1    @1 COCKCROFT (Robert)
A11 18  1    @1 COLLINS (MichelleL M.)
A11 19  1    @1 FARDAL (Mark A.)
A11 20  1    @1 HARRIS (William E.)
A11 21  1    @1 HUXOR (Avon)
A11 22  1    @1 MACKEY (A. Dougal)
A11 23  1    @1 PENARRUBIA (Jorge)
A11 24  1    @1 RICH (R. Michael)
A11 25  1    @1 RICHER (Harvey B.)
A11 26  1    @1 SIEBERT (Arnaud)
A11 27  1    @1 TANVIR (Nial)
A11 28  1    @1 VALLS-GABAUD (David)
A11 29  1    @1 VENN (Kimberly A.)
A14 01      @1 NRC Herzberg Institute of Astrophysics, 5071 West Saanich Road @2 Victoria, British Columbia, V9E 2E7 @3 CAN @Z 1 aut. @Z 7 aut. @Z 11 aut.
A14 02      @1 Institute of Astronomy, University of Cambridge, Madingley Road @2 Cambridge CB3 OHA @3 GBR @Z 2 aut. @Z 16 aut. @Z 18 aut. @Z 23 aut.
A14 03      @1 Observatoire de Strasbourg,11, rue de l'Université @2 67000 Strasbourg @3 FRA @Z 3 aut. @Z 15 aut. @Z 26 aut.
A14 04      @1 Department of Astronomy & Astrophysics, University of Toronto, 50 St George Street @2 Toronto, Ontario, M5S 3H4 @3 CAN @Z 4 aut.
A14 05      @1 Department of Physics, Engineering Physics, and Astronomy Queen's University @2 Kingston, Ontario, K7L 3N6 @3 CAN @Z 5 aut.
A14 06      @1 MaxPlanck-Institut für Astronomie, Königstuhl 17 @2 69117 Heidelberg @3 DEU @Z 6 aut.
A14 07      @1 Department of Physics and Astronomy, University of Victoria, 3800 Finnerty Road @2 Victoria, British Columbia, V8P 5C2 @3 CAN @Z 8 aut. @Z 9 aut. @Z 13 aut. @Z 29 aut.
A14 08      @1 Institute for Astronomy, University of Edinburgh, Royal Observatory, Blackford Hill @2 Edinburgh EH9 3HJ @3 GBR @Z 10 aut. @Z 22 aut.
A14 09      @1 Sydney Institute for Astronomy, School of Physics, University of Sydney @2 NSW 2006 @3 AUS @Z 12 aut.
A14 10      @1 Department of Physics and Astronomy, University of Western Ontario, 1151 Richmond Street @2 London, Ontario, N6A 3K7 @3 CAN @Z 14 aut.
A14 11      @1 Department of Physics and Astronomy, McMaster University @2 Hamilton, Ontario, L8S 4Ml @3 CAN @Z 17 aut. @Z 20 aut.
A14 12      @1 University of Massachusetts, Department of Astronomy, LGRT 619-E, 710 N. Pleasant Street @2 Amherst, Massachusetts 01003-9305 @3 USA @Z 19 aut.
A14 13      @1 Department of Physics (Astrophysics Group), H. H. Wills Physics Laboratory, Tyndall Avenue @2 Bristol BS81TL @3 GBR @Z 21 aut.
A14 14      @1 Department of Physics and Astronomy, University of California, Los Angeles, PAB, 430 Portola Plaza @2 Los Angeles, California 90095-1547 @3 USA @Z 24 aut.
A14 15      @1 Department of Physics and Astronomy, 6224 Agricultural Road, University of British Columbia @2 Vancouver, British Columbia, V6T 1Z1 @3 CAN @Z 25 aut.
A14 16      @1 Department of Physics and Astronomy, University of Leicester @2 Leicester LE1 7RH @3 GBR @Z 27 aut.
A14 17      @1 Laboratoire Galaxies et Étoiles, Physique et Instrumentation, CNRS UMR 8111, Observatoire de Paris, 5 Place Jules Janssen @2 92195 Meudon @3 FRA @Z 28 aut.
A20       @1 66-69
A21       @1 2009
A23 01      @0 ENG
A43 01      @1 INIST @2 142 @5 354000171844180110
A44       @0 0000 @1 © 2009 INIST-CNRS. All rights reserved.
A45       @0 30 ref.
A47 01  1    @0 09-0386067
A60       @1 P @3 CR
A61       @0 A
A64 01  1    @0 Nature : (London)
A66 01      @0 GBR
C01 01    ENG  @0 In hierarchical cosmological models', galaxies grow in mass through the continual accretion of smaller ones. The tidal disruption of these systems is expected to result in loosely bound stars surrounding the galaxy, at distances that reach 10-100 times the radius of the central disk2,3. The number, luminosity and morphology of the relics of this process provide significant clues to galaxy formation history4, but obtaining a comprehensive survey of these components is difficult because of their intrinsic faintness and vast extent. Here we report a panoramic survey of the Andromeda galaxy (M31). We detect stars and coherent structures that are almost certainly remnants of dwarf galaxies destroyed by the tidal field of M31. An improved census of their surviving counterparts implies that three-quarters of M31's satellites brighter than Mv = -6 await discovery. The brightest companion, Triangulum (M33), is surrounded by a stellar structure that provides persuasive evidence for a recent encounter with M31. This panorama of galaxy structure directly confirms the basic tenets of the hierarchical galaxy formation model and reveals the shared history of M31 and M33 in the unceasing build-up of galaxies.
C02 01  3    @0 001E03D62A
C03 01  3  FRE  @0 Formation galaxies @5 26
C03 01  3  ENG  @0 Galaxy formation @5 26
C03 02  3  FRE  @0 Modèle cosmologique @5 27
C03 02  3  ENG  @0 Cosmological models @5 27
C03 03  3  FRE  @0 Galaxies naines @5 28
C03 03  3  ENG  @0 Dwarf galaxies @5 28
C03 04  3  FRE  @0 Accrétion @5 29
C03 04  3  ENG  @0 Accretion @5 29
C03 05  3  FRE  @0 Luminosité @5 30
C03 05  3  ENG  @0 Luminosity @5 30
C03 06  3  FRE  @0 Morphologie @5 31
C03 06  3  ENG  @0 Morphology @5 31
C03 07  3  FRE  @0 Structure stellaire @5 32
C03 07  3  ENG  @0 Stellar structure @5 32
C03 08  X  FRE  @0 Structure galaxies @5 33
C03 08  X  ENG  @0 Galaxy structure @5 33
C03 08  X  SPA  @0 Estructura galaxias @5 33
C03 09  3  FRE  @0 Cosmologie @5 34
C03 09  3  ENG  @0 Cosmology @5 34
N21       @1 278

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Pascal:09-0386067

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<name sortKey="Cockcroft, Robert" sort="Cockcroft, Robert" uniqKey="Cockcroft R" first="Robert" last="Cockcroft">Robert Cockcroft</name>
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<s1>Department of Physics and Astronomy, McMaster University</s1>
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<name sortKey="Collins, Michellel M" sort="Collins, Michellel M" uniqKey="Collins M" first="Michellel M." last="Collins">Michellel M. Collins</name>
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<name sortKey="Fardal, Mark A" sort="Fardal, Mark A" uniqKey="Fardal M" first="Mark A." last="Fardal">Mark A. Fardal</name>
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<s1>University of Massachusetts, Department of Astronomy, LGRT 619-E, 710 N. Pleasant Street</s1>
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<name sortKey="Harris, William E" sort="Harris, William E" uniqKey="Harris W" first="William E." last="Harris">William E. Harris</name>
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<s1>Department of Physics and Astronomy, McMaster University</s1>
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<name sortKey="Huxor, Avon" sort="Huxor, Avon" uniqKey="Huxor A" first="Avon" last="Huxor">Avon Huxor</name>
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<s1>Department of Physics (Astrophysics Group), H. H. Wills Physics Laboratory, Tyndall Avenue</s1>
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<author>
<name sortKey="Mackey, A Dougal" sort="Mackey, A Dougal" uniqKey="Mackey A" first="A. Dougal" last="Mackey">A. Dougal Mackey</name>
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<inist:fA14 i1="08">
<s1>Institute for Astronomy, University of Edinburgh, Royal Observatory, Blackford Hill</s1>
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<author>
<name sortKey="Penarrubia, Jorge" sort="Penarrubia, Jorge" uniqKey="Penarrubia J" first="Jorge" last="Penarrubia">Jorge Penarrubia</name>
<affiliation wicri:level="1">
<inist:fA14 i1="02">
<s1>Institute of Astronomy, University of Cambridge, Madingley Road</s1>
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<author>
<name sortKey="Rich, R Michael" sort="Rich, R Michael" uniqKey="Rich R" first="R. Michael" last="Rich">R. Michael Rich</name>
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<inist:fA14 i1="14">
<s1>Department of Physics and Astronomy, University of California, Los Angeles, PAB, 430 Portola Plaza</s1>
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<author>
<name sortKey="Richer, Harvey B" sort="Richer, Harvey B" uniqKey="Richer H" first="Harvey B." last="Richer">Harvey B. Richer</name>
<affiliation wicri:level="1">
<inist:fA14 i1="15">
<s1>Department of Physics and Astronomy, 6224 Agricultural Road, University of British Columbia</s1>
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<s3>CAN</s3>
<sZ>25 aut.</sZ>
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<country>Canada</country>
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<author>
<name sortKey="Siebert, Arnaud" sort="Siebert, Arnaud" uniqKey="Siebert A" first="Arnaud" last="Siebert">Arnaud Siebert</name>
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<author>
<name sortKey="Tanvir, Nial" sort="Tanvir, Nial" uniqKey="Tanvir N" first="Nial" last="Tanvir">Nial Tanvir</name>
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</affiliation>
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<author>
<name sortKey="Valls Gabaud, David" sort="Valls Gabaud, David" uniqKey="Valls Gabaud D" first="David" last="Valls-Gabaud">David Valls-Gabaud</name>
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<s2>92195 Meudon</s2>
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</inist:fA14>
<country>France</country>
</affiliation>
</author>
<author>
<name sortKey="Venn, Kimberly A" sort="Venn, Kimberly A" uniqKey="Venn K" first="Kimberly A." last="Venn">Kimberly A. Venn</name>
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<inist:fA14 i1="07">
<s1>Department of Physics and Astronomy, University of Victoria, 3800 Finnerty Road</s1>
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</titleStmt>
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<idno type="inist">09-0386067</idno>
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<idno type="wicri:Area/PascalFrancis/Corpus">002B94</idno>
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<title xml:lang="en" level="a">The remnants of galaxy formation from a panoramic survey of the region around M31</title>
<author>
<name sortKey="Mcconnachie, Alan W" sort="Mcconnachie, Alan W" uniqKey="Mcconnachie A" first="Alan W." last="Mcconnachie">Alan W. Mcconnachie</name>
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<s1>NRC Herzberg Institute of Astrophysics, 5071 West Saanich Road</s1>
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<author>
<name sortKey="Irwin, Michael J" sort="Irwin, Michael J" uniqKey="Irwin M" first="Michael J." last="Irwin">Michael J. Irwin</name>
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<author>
<name sortKey="Dubinski, John" sort="Dubinski, John" uniqKey="Dubinski J" first="John" last="Dubinski">John Dubinski</name>
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<author>
<name sortKey="Widrow, Lawrence M" sort="Widrow, Lawrence M" uniqKey="Widrow L" first="Lawrence M." last="Widrow">Lawrence M. Widrow</name>
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<inist:fA14 i1="05">
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</inist:fA14>
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</author>
<author>
<name sortKey="Martin, Nicolas F" sort="Martin, Nicolas F" uniqKey="Martin N" first="Nicolas F." last="Martin">Nicolas F. Martin</name>
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<inist:fA14 i1="06">
<s1>MaxPlanck-Institut für Astronomie, Königstuhl 17</s1>
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<author>
<name sortKey="Cote, Patrick" sort="Cote, Patrick" uniqKey="Cote P" first="Patrick" last="Cote">Patrick Cote</name>
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<author>
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</affiliation>
</author>
<author>
<name sortKey="Navarro, Julio F" sort="Navarro, Julio F" uniqKey="Navarro J" first="Julio F." last="Navarro">Julio F. Navarro</name>
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</affiliation>
</author>
<author>
<name sortKey="Ferguson, Annette M N" sort="Ferguson, Annette M N" uniqKey="Ferguson A" first="Annette M. N." last="Ferguson">Annette M. N. Ferguson</name>
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<s1>Institute for Astronomy, University of Edinburgh, Royal Observatory, Blackford Hill</s1>
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<country>Royaume-Uni</country>
</affiliation>
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<author>
<name sortKey="Puzia, Thomas H" sort="Puzia, Thomas H" uniqKey="Puzia T" first="Thomas H." last="Puzia">Thomas H. Puzia</name>
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<inist:fA14 i1="01">
<s1>NRC Herzberg Institute of Astrophysics, 5071 West Saanich Road</s1>
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<name sortKey="Lewis, Geraint F" sort="Lewis, Geraint F" uniqKey="Lewis G" first="Geraint F." last="Lewis">Geraint F. Lewis</name>
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<inist:fA14 i1="09">
<s1>Sydney Institute for Astronomy, School of Physics, University of Sydney</s1>
<s2>NSW 2006</s2>
<s3>AUS</s3>
<sZ>12 aut.</sZ>
</inist:fA14>
<country>Australie</country>
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<name sortKey="Babu, Arif" sort="Babu, Arif" uniqKey="Babu A" first="Arif" last="Babu">Arif Babu</name>
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<s1>Department of Physics and Astronomy, University of Victoria, 3800 Finnerty Road</s1>
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<sZ>8 aut.</sZ>
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</affiliation>
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<author>
<name sortKey="Barmby, Pauline" sort="Barmby, Pauline" uniqKey="Barmby P" first="Pauline" last="Barmby">Pauline Barmby</name>
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<inist:fA14 i1="10">
<s1>Department of Physics and Astronomy, University of Western Ontario, 1151 Richmond Street</s1>
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<sZ>14 aut.</sZ>
</inist:fA14>
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</affiliation>
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<author>
<name sortKey="Bienayme, Olivier" sort="Bienayme, Olivier" uniqKey="Bienayme O" first="Olivier" last="Bienayme">Olivier Bienayme</name>
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<inist:fA14 i1="03">
<s1>Observatoire de Strasbourg,11, rue de l'Université</s1>
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</affiliation>
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<name sortKey="Chapman, Scott C" sort="Chapman, Scott C" uniqKey="Chapman S" first="Scott C." last="Chapman">Scott C. Chapman</name>
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<inist:fA14 i1="02">
<s1>Institute of Astronomy, University of Cambridge, Madingley Road</s1>
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</affiliation>
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<author>
<name sortKey="Cockcroft, Robert" sort="Cockcroft, Robert" uniqKey="Cockcroft R" first="Robert" last="Cockcroft">Robert Cockcroft</name>
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<inist:fA14 i1="11">
<s1>Department of Physics and Astronomy, McMaster University</s1>
<s2>Hamilton, Ontario, L8S 4Ml</s2>
<s3>CAN</s3>
<sZ>17 aut.</sZ>
<sZ>20 aut.</sZ>
</inist:fA14>
<country>Canada</country>
</affiliation>
</author>
<author>
<name sortKey="Collins, Michellel M" sort="Collins, Michellel M" uniqKey="Collins M" first="Michellel M." last="Collins">Michellel M. Collins</name>
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<inist:fA14 i1="02">
<s1>Institute of Astronomy, University of Cambridge, Madingley Road</s1>
<s2>Cambridge CB3 OHA</s2>
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</affiliation>
</author>
<author>
<name sortKey="Fardal, Mark A" sort="Fardal, Mark A" uniqKey="Fardal M" first="Mark A." last="Fardal">Mark A. Fardal</name>
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<inist:fA14 i1="12">
<s1>University of Massachusetts, Department of Astronomy, LGRT 619-E, 710 N. Pleasant Street</s1>
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<country>États-Unis</country>
</affiliation>
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<author>
<name sortKey="Harris, William E" sort="Harris, William E" uniqKey="Harris W" first="William E." last="Harris">William E. Harris</name>
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<inist:fA14 i1="11">
<s1>Department of Physics and Astronomy, McMaster University</s1>
<s2>Hamilton, Ontario, L8S 4Ml</s2>
<s3>CAN</s3>
<sZ>17 aut.</sZ>
<sZ>20 aut.</sZ>
</inist:fA14>
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</affiliation>
</author>
<author>
<name sortKey="Huxor, Avon" sort="Huxor, Avon" uniqKey="Huxor A" first="Avon" last="Huxor">Avon Huxor</name>
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<inist:fA14 i1="13">
<s1>Department of Physics (Astrophysics Group), H. H. Wills Physics Laboratory, Tyndall Avenue</s1>
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<s3>GBR</s3>
<sZ>21 aut.</sZ>
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<country>Royaume-Uni</country>
</affiliation>
</author>
<author>
<name sortKey="Mackey, A Dougal" sort="Mackey, A Dougal" uniqKey="Mackey A" first="A. Dougal" last="Mackey">A. Dougal Mackey</name>
<affiliation wicri:level="1">
<inist:fA14 i1="08">
<s1>Institute for Astronomy, University of Edinburgh, Royal Observatory, Blackford Hill</s1>
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<sZ>10 aut.</sZ>
<sZ>22 aut.</sZ>
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<country>Royaume-Uni</country>
</affiliation>
</author>
<author>
<name sortKey="Penarrubia, Jorge" sort="Penarrubia, Jorge" uniqKey="Penarrubia J" first="Jorge" last="Penarrubia">Jorge Penarrubia</name>
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<s1>Institute of Astronomy, University of Cambridge, Madingley Road</s1>
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<sZ>16 aut.</sZ>
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</affiliation>
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<author>
<name sortKey="Rich, R Michael" sort="Rich, R Michael" uniqKey="Rich R" first="R. Michael" last="Rich">R. Michael Rich</name>
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<inist:fA14 i1="14">
<s1>Department of Physics and Astronomy, University of California, Los Angeles, PAB, 430 Portola Plaza</s1>
<s2>Los Angeles, California 90095-1547</s2>
<s3>USA</s3>
<sZ>24 aut.</sZ>
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<country>États-Unis</country>
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<author>
<name sortKey="Richer, Harvey B" sort="Richer, Harvey B" uniqKey="Richer H" first="Harvey B." last="Richer">Harvey B. Richer</name>
<affiliation wicri:level="1">
<inist:fA14 i1="15">
<s1>Department of Physics and Astronomy, 6224 Agricultural Road, University of British Columbia</s1>
<s2>Vancouver, British Columbia, V6T 1Z1</s2>
<s3>CAN</s3>
<sZ>25 aut.</sZ>
</inist:fA14>
<country>Canada</country>
</affiliation>
</author>
<author>
<name sortKey="Siebert, Arnaud" sort="Siebert, Arnaud" uniqKey="Siebert A" first="Arnaud" last="Siebert">Arnaud Siebert</name>
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<inist:fA14 i1="03">
<s1>Observatoire de Strasbourg,11, rue de l'Université</s1>
<s2>67000 Strasbourg</s2>
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<sZ>3 aut.</sZ>
<sZ>15 aut.</sZ>
<sZ>26 aut.</sZ>
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<country>France</country>
</affiliation>
</author>
<author>
<name sortKey="Tanvir, Nial" sort="Tanvir, Nial" uniqKey="Tanvir N" first="Nial" last="Tanvir">Nial Tanvir</name>
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<inist:fA14 i1="16">
<s1>Department of Physics and Astronomy, University of Leicester</s1>
<s2>Leicester LE1 7RH</s2>
<s3>GBR</s3>
<sZ>27 aut.</sZ>
</inist:fA14>
<country>Royaume-Uni</country>
</affiliation>
</author>
<author>
<name sortKey="Valls Gabaud, David" sort="Valls Gabaud, David" uniqKey="Valls Gabaud D" first="David" last="Valls-Gabaud">David Valls-Gabaud</name>
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<inist:fA14 i1="17">
<s1>Laboratoire Galaxies et Étoiles, Physique et Instrumentation, CNRS UMR 8111, Observatoire de Paris, 5 Place Jules Janssen</s1>
<s2>92195 Meudon</s2>
<s3>FRA</s3>
<sZ>28 aut.</sZ>
</inist:fA14>
<country>France</country>
</affiliation>
</author>
<author>
<name sortKey="Venn, Kimberly A" sort="Venn, Kimberly A" uniqKey="Venn K" first="Kimberly A." last="Venn">Kimberly A. Venn</name>
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<inist:fA14 i1="07">
<s1>Department of Physics and Astronomy, University of Victoria, 3800 Finnerty Road</s1>
<s2>Victoria, British Columbia, V8P 5C2</s2>
<s3>CAN</s3>
<sZ>8 aut.</sZ>
<sZ>9 aut.</sZ>
<sZ>13 aut.</sZ>
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</affiliation>
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<series>
<title level="j" type="main">Nature : (London)</title>
<title level="j" type="abbreviated">Nature : (Lond.)</title>
<idno type="ISSN">0028-0836</idno>
<imprint>
<date when="2009">2009</date>
</imprint>
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<title level="j" type="main">Nature : (London)</title>
<title level="j" type="abbreviated">Nature : (Lond.)</title>
<idno type="ISSN">0028-0836</idno>
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<textClass>
<keywords scheme="KwdEn" xml:lang="en">
<term>Accretion</term>
<term>Cosmological models</term>
<term>Cosmology</term>
<term>Dwarf galaxies</term>
<term>Galaxy formation</term>
<term>Galaxy structure</term>
<term>Luminosity</term>
<term>Morphology</term>
<term>Stellar structure</term>
</keywords>
<keywords scheme="Pascal" xml:lang="fr">
<term>Formation galaxies</term>
<term>Modèle cosmologique</term>
<term>Galaxies naines</term>
<term>Accrétion</term>
<term>Luminosité</term>
<term>Morphologie</term>
<term>Structure stellaire</term>
<term>Structure galaxies</term>
<term>Cosmologie</term>
</keywords>
<keywords scheme="Wicri" type="topic" xml:lang="fr">
<term>Cosmologie</term>
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<front>
<div type="abstract" xml:lang="en">In hierarchical cosmological models', galaxies grow in mass through the continual accretion of smaller ones. The tidal disruption of these systems is expected to result in loosely bound stars surrounding the galaxy, at distances that reach 10-100 times the radius of the central disk
<sup>2,3</sup>
. The number, luminosity and morphology of the relics of this process provide significant clues to galaxy formation history
<sup>4</sup>
, but obtaining a comprehensive survey of these components is difficult because of their intrinsic faintness and vast extent. Here we report a panoramic survey of the Andromeda galaxy (M31). We detect stars and coherent structures that are almost certainly remnants of dwarf galaxies destroyed by the tidal field of M31. An improved census of their surviving counterparts implies that three-quarters of M31's satellites brighter than M
<sub>v</sub>
= -6 await discovery. The brightest companion, Triangulum (M33), is surrounded by a stellar structure that provides persuasive evidence for a recent encounter with M31. This panorama of galaxy structure directly confirms the basic tenets of the hierarchical galaxy formation model and reveals the shared history of M31 and M33 in the unceasing build-up of galaxies.</div>
</front>
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<s1>The remnants of galaxy formation from a panoramic survey of the region around M31</s1>
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<s1>MCCONNACHIE (Alan W.)</s1>
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<s1>IRWIN (Michael J.)</s1>
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<s1>IBATA (Rodrigo A.)</s1>
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<s1>DUBINSKI (John)</s1>
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<s1>WIDROW (Lawrence M.)</s1>
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<s1>MARTIN (Nicolas F.)</s1>
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<s1>COTE (Patrick)</s1>
</fA11>
<fA11 i1="08" i2="1">
<s1>DOTTER (Aaron L.)</s1>
</fA11>
<fA11 i1="09" i2="1">
<s1>NAVARRO (Julio F.)</s1>
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<s1>FERGUSON (Annette M. N.)</s1>
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<fA11 i1="11" i2="1">
<s1>PUZIA (Thomas H.)</s1>
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<s1>LEWIS (Geraint F.)</s1>
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<fA11 i1="13" i2="1">
<s1>BABU (Arif)</s1>
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<fA11 i1="14" i2="1">
<s1>BARMBY (Pauline)</s1>
</fA11>
<fA11 i1="15" i2="1">
<s1>BIENAYME (Olivier)</s1>
</fA11>
<fA11 i1="16" i2="1">
<s1>CHAPMAN (Scott C.)</s1>
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<s1>COCKCROFT (Robert)</s1>
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<fA11 i1="18" i2="1">
<s1>COLLINS (MichelleL M.)</s1>
</fA11>
<fA11 i1="19" i2="1">
<s1>FARDAL (Mark A.)</s1>
</fA11>
<fA11 i1="20" i2="1">
<s1>HARRIS (William E.)</s1>
</fA11>
<fA11 i1="21" i2="1">
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<fA11 i1="22" i2="1">
<s1>MACKEY (A. Dougal)</s1>
</fA11>
<fA11 i1="23" i2="1">
<s1>PENARRUBIA (Jorge)</s1>
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<s1>RICH (R. Michael)</s1>
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<fA11 i1="25" i2="1">
<s1>RICHER (Harvey B.)</s1>
</fA11>
<fA11 i1="26" i2="1">
<s1>SIEBERT (Arnaud)</s1>
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<fA11 i1="27" i2="1">
<s1>TANVIR (Nial)</s1>
</fA11>
<fA11 i1="28" i2="1">
<s1>VALLS-GABAUD (David)</s1>
</fA11>
<fA11 i1="29" i2="1">
<s1>VENN (Kimberly A.)</s1>
</fA11>
<fA14 i1="01">
<s1>NRC Herzberg Institute of Astrophysics, 5071 West Saanich Road</s1>
<s2>Victoria, British Columbia, V9E 2E7</s2>
<s3>CAN</s3>
<sZ>1 aut.</sZ>
<sZ>7 aut.</sZ>
<sZ>11 aut.</sZ>
</fA14>
<fA14 i1="02">
<s1>Institute of Astronomy, University of Cambridge, Madingley Road</s1>
<s2>Cambridge CB3 OHA</s2>
<s3>GBR</s3>
<sZ>2 aut.</sZ>
<sZ>16 aut.</sZ>
<sZ>18 aut.</sZ>
<sZ>23 aut.</sZ>
</fA14>
<fA14 i1="03">
<s1>Observatoire de Strasbourg,11, rue de l'Université</s1>
<s2>67000 Strasbourg</s2>
<s3>FRA</s3>
<sZ>3 aut.</sZ>
<sZ>15 aut.</sZ>
<sZ>26 aut.</sZ>
</fA14>
<fA14 i1="04">
<s1>Department of Astronomy & Astrophysics, University of Toronto, 50 St George Street</s1>
<s2>Toronto, Ontario, M5S 3H4</s2>
<s3>CAN</s3>
<sZ>4 aut.</sZ>
</fA14>
<fA14 i1="05">
<s1>Department of Physics, Engineering Physics, and Astronomy Queen's University</s1>
<s2>Kingston, Ontario, K7L 3N6</s2>
<s3>CAN</s3>
<sZ>5 aut.</sZ>
</fA14>
<fA14 i1="06">
<s1>MaxPlanck-Institut für Astronomie, Königstuhl 17</s1>
<s2>69117 Heidelberg</s2>
<s3>DEU</s3>
<sZ>6 aut.</sZ>
</fA14>
<fA14 i1="07">
<s1>Department of Physics and Astronomy, University of Victoria, 3800 Finnerty Road</s1>
<s2>Victoria, British Columbia, V8P 5C2</s2>
<s3>CAN</s3>
<sZ>8 aut.</sZ>
<sZ>9 aut.</sZ>
<sZ>13 aut.</sZ>
<sZ>29 aut.</sZ>
</fA14>
<fA14 i1="08">
<s1>Institute for Astronomy, University of Edinburgh, Royal Observatory, Blackford Hill</s1>
<s2>Edinburgh EH9 3HJ</s2>
<s3>GBR</s3>
<sZ>10 aut.</sZ>
<sZ>22 aut.</sZ>
</fA14>
<fA14 i1="09">
<s1>Sydney Institute for Astronomy, School of Physics, University of Sydney</s1>
<s2>NSW 2006</s2>
<s3>AUS</s3>
<sZ>12 aut.</sZ>
</fA14>
<fA14 i1="10">
<s1>Department of Physics and Astronomy, University of Western Ontario, 1151 Richmond Street</s1>
<s2>London, Ontario, N6A 3K7</s2>
<s3>CAN</s3>
<sZ>14 aut.</sZ>
</fA14>
<fA14 i1="11">
<s1>Department of Physics and Astronomy, McMaster University</s1>
<s2>Hamilton, Ontario, L8S 4Ml</s2>
<s3>CAN</s3>
<sZ>17 aut.</sZ>
<sZ>20 aut.</sZ>
</fA14>
<fA14 i1="12">
<s1>University of Massachusetts, Department of Astronomy, LGRT 619-E, 710 N. Pleasant Street</s1>
<s2>Amherst, Massachusetts 01003-9305</s2>
<s3>USA</s3>
<sZ>19 aut.</sZ>
</fA14>
<fA14 i1="13">
<s1>Department of Physics (Astrophysics Group), H. H. Wills Physics Laboratory, Tyndall Avenue</s1>
<s2>Bristol BS81TL</s2>
<s3>GBR</s3>
<sZ>21 aut.</sZ>
</fA14>
<fA14 i1="14">
<s1>Department of Physics and Astronomy, University of California, Los Angeles, PAB, 430 Portola Plaza</s1>
<s2>Los Angeles, California 90095-1547</s2>
<s3>USA</s3>
<sZ>24 aut.</sZ>
</fA14>
<fA14 i1="15">
<s1>Department of Physics and Astronomy, 6224 Agricultural Road, University of British Columbia</s1>
<s2>Vancouver, British Columbia, V6T 1Z1</s2>
<s3>CAN</s3>
<sZ>25 aut.</sZ>
</fA14>
<fA14 i1="16">
<s1>Department of Physics and Astronomy, University of Leicester</s1>
<s2>Leicester LE1 7RH</s2>
<s3>GBR</s3>
<sZ>27 aut.</sZ>
</fA14>
<fA14 i1="17">
<s1>Laboratoire Galaxies et Étoiles, Physique et Instrumentation, CNRS UMR 8111, Observatoire de Paris, 5 Place Jules Janssen</s1>
<s2>92195 Meudon</s2>
<s3>FRA</s3>
<sZ>28 aut.</sZ>
</fA14>
<fA20>
<s1>66-69</s1>
</fA20>
<fA21>
<s1>2009</s1>
</fA21>
<fA23 i1="01">
<s0>ENG</s0>
</fA23>
<fA43 i1="01">
<s1>INIST</s1>
<s2>142</s2>
<s5>354000171844180110</s5>
</fA43>
<fA44>
<s0>0000</s0>
<s1>© 2009 INIST-CNRS. All rights reserved.</s1>
</fA44>
<fA45>
<s0>30 ref.</s0>
</fA45>
<fA47 i1="01" i2="1">
<s0>09-0386067</s0>
</fA47>
<fA60>
<s1>P</s1>
<s3>CR</s3>
</fA60>
<fA61>
<s0>A</s0>
</fA61>
<fA64 i1="01" i2="1">
<s0>Nature : (London)</s0>
</fA64>
<fA66 i1="01">
<s0>GBR</s0>
</fA66>
<fC01 i1="01" l="ENG">
<s0>In hierarchical cosmological models', galaxies grow in mass through the continual accretion of smaller ones. The tidal disruption of these systems is expected to result in loosely bound stars surrounding the galaxy, at distances that reach 10-100 times the radius of the central disk
<sup>2,3</sup>
. The number, luminosity and morphology of the relics of this process provide significant clues to galaxy formation history
<sup>4</sup>
, but obtaining a comprehensive survey of these components is difficult because of their intrinsic faintness and vast extent. Here we report a panoramic survey of the Andromeda galaxy (M31). We detect stars and coherent structures that are almost certainly remnants of dwarf galaxies destroyed by the tidal field of M31. An improved census of their surviving counterparts implies that three-quarters of M31's satellites brighter than M
<sub>v</sub>
= -6 await discovery. The brightest companion, Triangulum (M33), is surrounded by a stellar structure that provides persuasive evidence for a recent encounter with M31. This panorama of galaxy structure directly confirms the basic tenets of the hierarchical galaxy formation model and reveals the shared history of M31 and M33 in the unceasing build-up of galaxies.</s0>
</fC01>
<fC02 i1="01" i2="3">
<s0>001E03D62A</s0>
</fC02>
<fC03 i1="01" i2="3" l="FRE">
<s0>Formation galaxies</s0>
<s5>26</s5>
</fC03>
<fC03 i1="01" i2="3" l="ENG">
<s0>Galaxy formation</s0>
<s5>26</s5>
</fC03>
<fC03 i1="02" i2="3" l="FRE">
<s0>Modèle cosmologique</s0>
<s5>27</s5>
</fC03>
<fC03 i1="02" i2="3" l="ENG">
<s0>Cosmological models</s0>
<s5>27</s5>
</fC03>
<fC03 i1="03" i2="3" l="FRE">
<s0>Galaxies naines</s0>
<s5>28</s5>
</fC03>
<fC03 i1="03" i2="3" l="ENG">
<s0>Dwarf galaxies</s0>
<s5>28</s5>
</fC03>
<fC03 i1="04" i2="3" l="FRE">
<s0>Accrétion</s0>
<s5>29</s5>
</fC03>
<fC03 i1="04" i2="3" l="ENG">
<s0>Accretion</s0>
<s5>29</s5>
</fC03>
<fC03 i1="05" i2="3" l="FRE">
<s0>Luminosité</s0>
<s5>30</s5>
</fC03>
<fC03 i1="05" i2="3" l="ENG">
<s0>Luminosity</s0>
<s5>30</s5>
</fC03>
<fC03 i1="06" i2="3" l="FRE">
<s0>Morphologie</s0>
<s5>31</s5>
</fC03>
<fC03 i1="06" i2="3" l="ENG">
<s0>Morphology</s0>
<s5>31</s5>
</fC03>
<fC03 i1="07" i2="3" l="FRE">
<s0>Structure stellaire</s0>
<s5>32</s5>
</fC03>
<fC03 i1="07" i2="3" l="ENG">
<s0>Stellar structure</s0>
<s5>32</s5>
</fC03>
<fC03 i1="08" i2="X" l="FRE">
<s0>Structure galaxies</s0>
<s5>33</s5>
</fC03>
<fC03 i1="08" i2="X" l="ENG">
<s0>Galaxy structure</s0>
<s5>33</s5>
</fC03>
<fC03 i1="08" i2="X" l="SPA">
<s0>Estructura galaxias</s0>
<s5>33</s5>
</fC03>
<fC03 i1="09" i2="3" l="FRE">
<s0>Cosmologie</s0>
<s5>34</s5>
</fC03>
<fC03 i1="09" i2="3" l="ENG">
<s0>Cosmology</s0>
<s5>34</s5>
</fC03>
<fN21>
<s1>278</s1>
</fN21>
</pA>
</standard>
</inist>
</record>

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