AustralieFrV1, PascalFrancis, Corpus, bibRecord, 004803

Internal alignment of the halos of disk galaxies in cosmological hydrodynamic simulations

Identifieur interne : 004803 ( PascalFrancis/Corpus ); précédent : 004802; suivant : 004804

Internal alignment of the halos of disk galaxies in cosmological hydrodynamic simulations

Auteurs : Jeremy Bailin ; Daisuke Kawata ; Brad K. Gibson ; Matthias Steinmetz ; Julio F. Navarro ; Chris B. Brook ; Stuart P. D. Gill ; Rodrigo A. Ibata ; Alexander Knebe ; Geraint F. Lewis ; Takashi Okamoto

Source :

The Astrophysical journal [ 0004-637X ] ; 2005.

RBID : Pascal:05-0382346

Descripteurs français

Pascal (Inist)
- Alignement, Galaxies disques, Modèle hydrodynamique, Simulation numérique, Matière sombre, Formation galaxies, Galaxies spirales, Halo galaxies, Evolution galaxies.

English descriptors

KwdEn :
- Alignment, Dark matter, Digital simulation, Disk galaxies, Galaxy evolution, Galaxy formation, Galaxy halo, Hydrodynamic model, Spiral galaxies.

Notice en format standard (ISO 2709)

Pour connaître la documentation sur le format Inist Standard.

A01	`01`	`1`		`@0 0004-637X`
A02	`01`			`@0 ASJOAB`
A03		`1`		`@0 Astrophys. j.`
A05				`@2 627`
A06				`@2 1 @3 p.2`
A08	`01`	`1`	`ENG`	`@1 Internal alignment of the halos of disk galaxies in cosmological hydrodynamic simulations`
A11	`01`	`1`		`@1 BAILIN (Jeremy)`
A11	`02`	`1`		`@1 KAWATA (Daisuke)`
A11	`03`	`1`		`@1 GIBSON (Brad K.)`
A11	`04`	`1`		`@1 STEINMETZ (Matthias)`
A11	`05`	`1`		`@1 NAVARRO (Julio F.)`
A11	`06`	`1`		`@1 BROOK (Chris B.)`
A11	`07`	`1`		`@1 GILL (Stuart P. D.)`
A11	`08`	`1`		`@1 IBATA (Rodrigo A.)`
A11	`09`	`1`		`@1 KNEBE (Alexander)`
A11	`10`	`1`		`@1 LEWIS (Geraint F.)`
A11	`11`	`1`		`@1 OKAMOTO (Takashi)`
A14	`01`			`@1 Centre for Astrophysics and Supercomputing, Swinburne University of Technology, P.O. Box 218 @2 Hawthorn, VIC 3122 @3 AUS @Z 1 aut. @Z 2 aut. @Z 3 aut. @Z 7 aut. @Z 9 aut.`
A14	`02`			`@1 Carnegie Observatories, 813 Santa Barbara Street @2 Pasadena, CA 91101 @3 USA @Z 2 aut.`
A14	`03`			`@1 Astrophysikalisches Institut Potsdam, An der Sternwarte 16 @2 14482 Potsdam @3 DEU @Z 4 aut. @Z 9 aut.`
A14	`04`			`@1 Department of Physics and Astronomy, University of Victoria, P.O. Box 3055, Station CSC @2 Victoria, BC V8W 3P6 @3 CAN @Z 5 aut.`
A14	`05`			`@1 Département de Physique, de Génie Physique et d'Optique. Université Laval @2 Québec, QC G1K 7P4 @3 CAN @Z 6 aut.`
A14	`06`			`@1 Observatoire de Strasbourg, 11 rue de l'Universite @2 67000 Strasbourg @3 FRA @Z 8 aut.`
A14	`07`			`@1 School of Physics, University of Sydney @2 NSW 2006 @3 AUS @Z 10 aut.`
A14	`08`			`@1 Institute for Computational Cosmology, Department of Physics, Durham University, South Road @2 Durham DH1 3LE @3 GBR @Z 11 aut.`
A14	`09`			`@1 National Astronomical Observatory of Japan, 2-21-1 Osawa @2 Mitaka, Tokyo 181-8588 @3 JPN @Z 11 aut.`
A20				`@2 L17-L20`
A21				`@1 2005`
A23	`01`			`@0 ENG`
A43	`01`			`@1 INIST @2 512 @5 354000138452100050`
A44				`@0 0000 @1 © 2005 INIST-CNRS. All rights reserved.`
A45				`@0 47 ref.`
A47	`01`	`1`		`@0 05-0382346`
A60				`@1 P`
A61				`@0 A`
A64	`01`	`1`		`@0 The Astrophysical journal`
A66	`01`			`@0 USA`
C02	`01`	`3`		`@0 001E03`
C03	`01`	`3`	`FRE`	`@0 Alignement @5 26`
C03	`01`	`3`	`ENG`	`@0 Alignment @5 26`
C03	`02`	`3`	`FRE`	`@0 Galaxies disques @5 27`
C03	`02`	`3`	`ENG`	`@0 Disk galaxies @5 27`
C03	`03`	`3`	`FRE`	`@0 Modèle hydrodynamique @5 28`
C03	`03`	`3`	`ENG`	`@0 Hydrodynamic model @5 28`
C03	`04`	`3`	`FRE`	`@0 Simulation numérique @5 29`
C03	`04`	`3`	`ENG`	`@0 Digital simulation @5 29`
C03	`05`	`3`	`FRE`	`@0 Matière sombre @5 30`
C03	`05`	`3`	`ENG`	`@0 Dark matter @5 30`
C03	`06`	`3`	`FRE`	`@0 Formation galaxies @5 31`
C03	`06`	`3`	`ENG`	`@0 Galaxy formation @5 31`
C03	`07`	`3`	`FRE`	`@0 Galaxies spirales @5 32`
C03	`07`	`3`	`ENG`	`@0 Spiral galaxies @5 32`
C03	`08`	`3`	`FRE`	`@0 Halo galaxies @4 CD @5 96`
C03	`08`	`3`	`ENG`	`@0 Galaxy halo @4 CD @5 96`
C03	`08`	`3`	`SPA`	`@0 Halo galaxia @4 CD @5 96`
C03	`09`	`3`	`FRE`	`@0 Evolution galaxies @4 CD @5 97`
C03	`09`	`3`	`ENG`	`@0 Galaxy evolution @4 CD @5 97`
C03	`09`	`3`	`SPA`	`@0 Evolución galaxias @4 CD @5 97`
N21				`@1 269`
N44	`01`			`@1 OTO`
N82				`@1 OTO`

Format Inist (serveur)

NO :	PASCAL 05-0382346 INIST
ET :	Internal alignment of the halos of disk galaxies in cosmological hydrodynamic simulations
AU :	BAILIN (Jeremy); KAWATA (Daisuke); GIBSON (Brad K.); STEINMETZ (Matthias); NAVARRO (Julio F.); BROOK (Chris B.); GILL (Stuart P. D.); IBATA (Rodrigo A.); KNEBE (Alexander); LEWIS (Geraint F.); OKAMOTO (Takashi)
AF :	Centre for Astrophysics and Supercomputing, Swinburne University of Technology, P.O. Box 218/Hawthorn, VIC 3122/Australie (1 aut., 2 aut., 3 aut., 7 aut., 9 aut.); Carnegie Observatories, 813 Santa Barbara Street/Pasadena, CA 91101/Etats-Unis (2 aut.); Astrophysikalisches Institut Potsdam, An der Sternwarte 16/14482 Potsdam/Allemagne (4 aut., 9 aut.); Department of Physics and Astronomy, University of Victoria, P.O. Box 3055, Station CSC/Victoria, BC V8W 3P6/Canada (5 aut.); Département de Physique, de Génie Physique et d'Optique. Université Laval/Québec, QC G1K 7P4/Canada (6 aut.); Observatoire de Strasbourg, 11 rue de l'Universite/67000 Strasbourg/France (8 aut.); School of Physics, University of Sydney/NSW 2006/Australie (10 aut.); Institute for Computational Cosmology, Department of Physics, Durham University, South Road/Durham DH1 3LE/Royaume-Uni (11 aut.); National Astronomical Observatory of Japan, 2-21-1 Osawa/Mitaka, Tokyo 181-8588/Japon (11 aut.)
DT :	Publication en série; Niveau analytique
SO :	The Astrophysical journal; ISSN 0004-637X; Coden ASJOAB; Etats-Unis; Da. 2005; Vol. 627; No. 1 p.2; L17-L20; Bibl. 47 ref.
LA :	Anglais
CC :	001E03
FD :	Alignement; Galaxies disques; Modèle hydrodynamique; Simulation numérique; Matière sombre; Formation galaxies; Galaxies spirales; Halo galaxies; Evolution galaxies
ED :	Alignment; Disk galaxies; Hydrodynamic model; Digital simulation; Dark matter; Galaxy formation; Spiral galaxies; Galaxy halo; Galaxy evolution
SD :	Halo galaxia; Evolución galaxias
LO :	INIST-512.354000138452100050
ID :	05-0382346

Links to Exploration step

Pascal:05-0382346

Le document en format XML

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<sourceDesc><biblStruct><analytic><title xml:lang="en" level="a">Internal alignment of the halos of disk galaxies in cosmological hydrodynamic simulations</title>
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<author><name sortKey="Gill, Stuart P D" sort="Gill, Stuart P D" uniqKey="Gill S" first="Stuart P. D." last="Gill">Stuart P. D. Gill</name>
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<author><name sortKey="Ibata, Rodrigo A" sort="Ibata, Rodrigo A" uniqKey="Ibata R" first="Rodrigo A." last="Ibata">Rodrigo A. Ibata</name>
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<author><name sortKey="Okamoto, Takashi" sort="Okamoto, Takashi" uniqKey="Okamoto T" first="Takashi" last="Okamoto">Takashi Okamoto</name>
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<series><title level="j" type="main">The Astrophysical journal</title>
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<profileDesc><textClass><keywords scheme="KwdEn" xml:lang="en"><term>Alignment</term>
<term>Dark matter</term>
<term>Digital simulation</term>
<term>Disk galaxies</term>
<term>Galaxy evolution</term>
<term>Galaxy formation</term>
<term>Galaxy halo</term>
<term>Hydrodynamic model</term>
<term>Spiral galaxies</term>
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<term>Galaxies disques</term>
<term>Modèle hydrodynamique</term>
<term>Simulation numérique</term>
<term>Matière sombre</term>
<term>Formation galaxies</term>
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<fA11 i1="01" i2="1"><s1>BAILIN (Jeremy)</s1>
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<fA11 i1="02" i2="1"><s1>KAWATA (Daisuke)</s1>
</fA11>
<fA11 i1="03" i2="1"><s1>GIBSON (Brad K.)</s1>
</fA11>
<fA11 i1="04" i2="1"><s1>STEINMETZ (Matthias)</s1>
</fA11>
<fA11 i1="05" i2="1"><s1>NAVARRO (Julio F.)</s1>
</fA11>
<fA11 i1="06" i2="1"><s1>BROOK (Chris B.)</s1>
</fA11>
<fA11 i1="07" i2="1"><s1>GILL (Stuart P. D.)</s1>
</fA11>
<fA11 i1="08" i2="1"><s1>IBATA (Rodrigo A.)</s1>
</fA11>
<fA11 i1="09" i2="1"><s1>KNEBE (Alexander)</s1>
</fA11>
<fA11 i1="10" i2="1"><s1>LEWIS (Geraint F.)</s1>
</fA11>
<fA11 i1="11" i2="1"><s1>OKAMOTO (Takashi)</s1>
</fA11>
<fA14 i1="01"><s1>Centre for Astrophysics and Supercomputing, Swinburne University of Technology, P.O. Box 218</s1>
<s2>Hawthorn, VIC 3122</s2>
<s3>AUS</s3>
<sZ>1 aut.</sZ>
<sZ>2 aut.</sZ>
<sZ>3 aut.</sZ>
<sZ>7 aut.</sZ>
<sZ>9 aut.</sZ>
</fA14>
<fA14 i1="02"><s1>Carnegie Observatories, 813 Santa Barbara Street</s1>
<s2>Pasadena, CA 91101</s2>
<s3>USA</s3>
<sZ>2 aut.</sZ>
</fA14>
<fA14 i1="03"><s1>Astrophysikalisches Institut Potsdam, An der Sternwarte 16</s1>
<s2>14482 Potsdam</s2>
<s3>DEU</s3>
<sZ>4 aut.</sZ>
<sZ>9 aut.</sZ>
</fA14>
<fA14 i1="04"><s1>Department of Physics and Astronomy, University of Victoria, P.O. Box 3055, Station CSC</s1>
<s2>Victoria, BC V8W 3P6</s2>
<s3>CAN</s3>
<sZ>5 aut.</sZ>
</fA14>
<fA14 i1="05"><s1>Département de Physique, de Génie Physique et d'Optique. Université Laval</s1>
<s2>Québec, QC G1K 7P4</s2>
<s3>CAN</s3>
<sZ>6 aut.</sZ>
</fA14>
<fA14 i1="06"><s1>Observatoire de Strasbourg, 11 rue de l'Universite</s1>
<s2>67000 Strasbourg</s2>
<s3>FRA</s3>
<sZ>8 aut.</sZ>
</fA14>
<fA14 i1="07"><s1>School of Physics, University of Sydney</s1>
<s2>NSW 2006</s2>
<s3>AUS</s3>
<sZ>10 aut.</sZ>
</fA14>
<fA14 i1="08"><s1>Institute for Computational Cosmology, Department of Physics, Durham University, South Road</s1>
<s2>Durham DH1 3LE</s2>
<s3>GBR</s3>
<sZ>11 aut.</sZ>
</fA14>
<fA14 i1="09"><s1>National Astronomical Observatory of Japan, 2-21-1 Osawa</s1>
<s2>Mitaka, Tokyo 181-8588</s2>
<s3>JPN</s3>
<sZ>11 aut.</sZ>
</fA14>
<fA20><s2>L17-L20</s2>
</fA20>
<fA21><s1>2005</s1>
</fA21>
<fA23 i1="01"><s0>ENG</s0>
</fA23>
<fA43 i1="01"><s1>INIST</s1>
<s2>512</s2>
<s5>354000138452100050</s5>
</fA43>
<fA44><s0>0000</s0>
<s1>© 2005 INIST-CNRS. All rights reserved.</s1>
</fA44>
<fA45><s0>47 ref.</s0>
</fA45>
<fA47 i1="01" i2="1"><s0>05-0382346</s0>
</fA47>
<fA60><s1>P</s1>
</fA60>
<fA61><s0>A</s0>
</fA61>
<fA64 i1="01" i2="1"><s0>The Astrophysical journal</s0>
</fA64>
<fA66 i1="01"><s0>USA</s0>
</fA66>
<fC02 i1="01" i2="3"><s0>001E03</s0>
</fC02>
<fC03 i1="01" i2="3" l="FRE"><s0>Alignement</s0>
<s5>26</s5>
</fC03>
<fC03 i1="01" i2="3" l="ENG"><s0>Alignment</s0>
<s5>26</s5>
</fC03>
<fC03 i1="02" i2="3" l="FRE"><s0>Galaxies disques</s0>
<s5>27</s5>
</fC03>
<fC03 i1="02" i2="3" l="ENG"><s0>Disk galaxies</s0>
<s5>27</s5>
</fC03>
<fC03 i1="03" i2="3" l="FRE"><s0>Modèle hydrodynamique</s0>
<s5>28</s5>
</fC03>
<fC03 i1="03" i2="3" l="ENG"><s0>Hydrodynamic model</s0>
<s5>28</s5>
</fC03>
<fC03 i1="04" i2="3" l="FRE"><s0>Simulation numérique</s0>
<s5>29</s5>
</fC03>
<fC03 i1="04" i2="3" l="ENG"><s0>Digital simulation</s0>
<s5>29</s5>
</fC03>
<fC03 i1="05" i2="3" l="FRE"><s0>Matière sombre</s0>
<s5>30</s5>
</fC03>
<fC03 i1="05" i2="3" l="ENG"><s0>Dark matter</s0>
<s5>30</s5>
</fC03>
<fC03 i1="06" i2="3" l="FRE"><s0>Formation galaxies</s0>
<s5>31</s5>
</fC03>
<fC03 i1="06" i2="3" l="ENG"><s0>Galaxy formation</s0>
<s5>31</s5>
</fC03>
<fC03 i1="07" i2="3" l="FRE"><s0>Galaxies spirales</s0>
<s5>32</s5>
</fC03>
<fC03 i1="07" i2="3" l="ENG"><s0>Spiral galaxies</s0>
<s5>32</s5>
</fC03>
<fC03 i1="08" i2="3" l="FRE"><s0>Halo galaxies</s0>
<s4>CD</s4>
<s5>96</s5>
</fC03>
<fC03 i1="08" i2="3" l="ENG"><s0>Galaxy halo</s0>
<s4>CD</s4>
<s5>96</s5>
</fC03>
<fC03 i1="08" i2="3" l="SPA"><s0>Halo galaxia</s0>
<s4>CD</s4>
<s5>96</s5>
</fC03>
<fC03 i1="09" i2="3" l="FRE"><s0>Evolution galaxies</s0>
<s4>CD</s4>
<s5>97</s5>
</fC03>
<fC03 i1="09" i2="3" l="ENG"><s0>Galaxy evolution</s0>
<s4>CD</s4>
<s5>97</s5>
</fC03>
<fC03 i1="09" i2="3" l="SPA"><s0>Evolución galaxias</s0>
<s4>CD</s4>
<s5>97</s5>
</fC03>
<fN21><s1>269</s1>
</fN21>
<fN44 i1="01"><s1>OTO</s1>
</fN44>
<fN82><s1>OTO</s1>
</fN82>
</pA>
</standard>
<server><NO>PASCAL 05-0382346 INIST</NO>
<ET>Internal alignment of the halos of disk galaxies in cosmological hydrodynamic simulations</ET>
<AU>BAILIN (Jeremy); KAWATA (Daisuke); GIBSON (Brad K.); STEINMETZ (Matthias); NAVARRO (Julio F.); BROOK (Chris B.); GILL (Stuart P. D.); IBATA (Rodrigo A.); KNEBE (Alexander); LEWIS (Geraint F.); OKAMOTO (Takashi)</AU>
<AF>Centre for Astrophysics and Supercomputing, Swinburne University of Technology, P.O. Box 218/Hawthorn, VIC 3122/Australie (1 aut., 2 aut., 3 aut., 7 aut., 9 aut.); Carnegie Observatories, 813 Santa Barbara Street/Pasadena, CA 91101/Etats-Unis (2 aut.); Astrophysikalisches Institut Potsdam, An der Sternwarte 16/14482 Potsdam/Allemagne (4 aut., 9 aut.); Department of Physics and Astronomy, University of Victoria, P.O. Box 3055, Station CSC/Victoria, BC V8W 3P6/Canada (5 aut.); Département de Physique, de Génie Physique et d'Optique. Université Laval/Québec, QC G1K 7P4/Canada (6 aut.); Observatoire de Strasbourg, 11 rue de l'Universite/67000 Strasbourg/France (8 aut.); School of Physics, University of Sydney/NSW 2006/Australie (10 aut.); Institute for Computational Cosmology, Department of Physics, Durham University, South Road/Durham DH1 3LE/Royaume-Uni (11 aut.); National Astronomical Observatory of Japan, 2-21-1 Osawa/Mitaka, Tokyo 181-8588/Japon (11 aut.)</AF>
<DT>Publication en série; Niveau analytique</DT>
<SO>The Astrophysical journal; ISSN 0004-637X; Coden ASJOAB; Etats-Unis; Da. 2005; Vol. 627; No. 1 p.2; L17-L20; Bibl. 47 ref.</SO>
<LA>Anglais</LA>
<CC>001E03</CC>
<FD>Alignement; Galaxies disques; Modèle hydrodynamique; Simulation numérique; Matière sombre; Formation galaxies; Galaxies spirales; Halo galaxies; Evolution galaxies</FD>
<ED>Alignment; Disk galaxies; Hydrodynamic model; Digital simulation; Dark matter; Galaxy formation; Spiral galaxies; Galaxy halo; Galaxy evolution</ED>
<SD>Halo galaxia; Evolución galaxias</SD>
<LO>INIST-512.354000138452100050</LO>
<ID>05-0382346</ID>
</server>
</inist>
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Internal alignment of the halos of disk galaxies in cosmological hydrodynamic simulations

Internal alignment of the halos of disk galaxies in cosmological hydrodynamic simulations

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