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The Herschel* Exploitation of Local Galaxy Andromeda (HELGA) I. Global far-infrared and sub-mm morphology

Identifieur interne : 005847 ( Main/Exploration ); précédent : 005846; suivant : 005848

The Herschel* Exploitation of Local Galaxy Andromeda (HELGA) I. Global far-infrared and sub-mm morphology

Auteurs : J. Fritz [Belgique] ; G. Gentile [Belgique] ; M. W. L. Smith [Royaume-Uni] ; W. K. Gear [Royaume-Uni] ; R. Braun [Australie] ; J. Roman Duval [États-Unis] ; G. J. Bendo [Royaume-Uni] ; M. Baes [Belgique] ; S. A. Eales [Royaume-Uni] ; J. Verstappen [Belgique] ; J. A. D. L. Blommaert [Belgique] ; M. Boquien [États-Unis, France] ; A. Boselli [France] ; D. Clements [Royaume-Uni] ; A. R. Cooray [États-Unis] ; L. Cortese [Allemagne] ; I. De Looze [Belgique] ; G. P. Ford [Royaume-Uni] ; F. Galliano [France] ; H. L. Gomez [Royaume-Uni] ; K. D. Gordon [Belgique, États-Unis] ; V. Lebouteiller [France] ; B. O'Halloran [Royaume-Uni] ; J. Kirk [Royaume-Uni] ; S. C. Madden [France] ; M. J. Page [Royaume-Uni] ; A. Remy [France] ; H. Roussel [France] ; L. Spinoglio [Italie] ; D. Thilker [États-Unis] ; M. Vaccari [Afrique du Sud] ; C. D. Wilson [Canada] ; C. Waelkens [Belgique]

Source :

RBID : Pascal:13-0044989

Descripteurs français

English descriptors

Abstract

Context. We have obtained Herschel images at five wavelengths from 100 to 500 μm of a ∼5.5 x 2.5 degree area centred on the local galaxy M 31 (Andromeda), our nearest neighbour spiral galaxy, as part of the Herschel guaranteed time project "HELGA". The main goals of HELGA are to study the characteristics of the extended dust emission, focusing on larger scales than studied in previous observations of Andromeda at an increased spatial resolution, and the obscured star formation. Aims. In this paper we present data reduction and Herschel maps, and provide a description of the far-infrared morphology, comparing it with features seen at other wavelengths. Methods. We used high-resolution maps of the atomic hydrogen, fully covering our fields, to identify dust emission features that can be associated to M 31 with confidence, distinguishing them from emission coming from the foreground Galactic cirrus. Results. Thanks to the very large extension of our maps we detect, for the first time at far-infrared wavelengths, three arc-like structures extending out to ∼21, ∼26 and ∼31 kpc respectively, in the south-western part of M 31. The presence of these features, hosting ∼2.2 x 106 M◦. of dust, is safely confirmed by their detection in HI maps. Overall, we estimate a total dust mass of ∼5.8 x 107 M◦., about 78% of which is contained in the two main ring-like structures at 10 and 15 kpc, at an average temperature of 16.5 K. We find that the gas-to-dust ratio declines exponentially as a function of the galacto-centric distance, in agreement with the known metallicity gradient, with values ranging from 66 in the nucleus to ∼275 in the outermost region. Conclusions. Dust in M31 extends significantly beyond its optical radius (∼21 kpc) and what was previously mapped in the far-infrared. An annular-like segment, located approximately at R25, is clearly detected on both sides of the galaxy, and two other similar annular structures are undoubtedly detected on the south-west side even further out.


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<title xml:lang="en" level="a">The Herschel
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Exploitation of Local Galaxy Andromeda (HELGA) I. Global far-infrared and sub-mm morphology</title>
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<s1>Sterrenkundig Observatorium, Universiteit Gent, Krijgslaan 281</s1>
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<s1>Sterrenkundig Observatorium, Universiteit Gent, Krijgslaan 281</s1>
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<wicri:noRegion>bâtiment 709</wicri:noRegion>
<wicri:noRegion>91191 Gif-sur-Yvette</wicri:noRegion>
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<name sortKey="Page, M J" sort="Page, M J" uniqKey="Page M" first="M. J." last="Page">M. J. Page</name>
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<s1>Mullard Space Science Laboratory, University College London, Holmbury St. Mary</s1>
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<country>Royaume-Uni</country>
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<region type="country">Angleterre</region>
<region type="région" nuts="1">Grand Londres</region>
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<s1>AIM, CEA/Saclay, Orme des Merisiers, bâtiment 709</s1>
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<placeName>
<region type="region" nuts="2">Île-de-France</region>
<settlement type="city">Gif-sur-Yvette</settlement>
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<name sortKey="Roussel, H" sort="Roussel, H" uniqKey="Roussel H" first="H." last="Roussel">H. Roussel</name>
<affiliation wicri:level="3">
<inist:fA14 i1="14">
<s1>Institut d'Astrophysique de Paris, UMR 7095 CNRS, Université Pierre & Marie Curie, 98bis boulevard Arago</s1>
<s2>75014 Paris</s2>
<s3>FRA</s3>
<sZ>28 aut.</sZ>
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<country>France</country>
<placeName>
<region type="region" nuts="2">Île-de-France</region>
<settlement type="city">Paris</settlement>
</placeName>
</affiliation>
</author>
<author>
<name sortKey="Spinoglio, L" sort="Spinoglio, L" uniqKey="Spinoglio L" first="L." last="Spinoglio">L. Spinoglio</name>
<affiliation wicri:level="1">
<inist:fA14 i1="15">
<s1>Istituto di Fisica dello Spazio Interplanetario, INAF, via Fosso del Cavaliere 100</s1>
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<s3>ITA</s3>
<sZ>29 aut.</sZ>
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<country>Italie</country>
<placeName>
<settlement type="city">Rome</settlement>
<region nuts="2">Latium</region>
</placeName>
</affiliation>
</author>
<author>
<name sortKey="Thilker, D" sort="Thilker, D" uniqKey="Thilker D" first="D." last="Thilker">D. Thilker</name>
<affiliation wicri:level="1">
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<s1>Dept. of Physics & Astronomy, Johns Hopkins University, 3400 N. Charles St.</s1>
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<s3>USA</s3>
<sZ>30 aut.</sZ>
</inist:fA14>
<country>États-Unis</country>
<wicri:noRegion>Baltimore, MD 21218</wicri:noRegion>
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</author>
<author>
<name sortKey="Vaccari, M" sort="Vaccari, M" uniqKey="Vaccari M" first="M." last="Vaccari">M. Vaccari</name>
<affiliation wicri:level="1">
<inist:fA14 i1="17">
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<s2>Bellville, 7535 Cape Town</s2>
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</inist:fA14>
<country>Afrique du Sud</country>
<wicri:noRegion>University of the Western Cape Private Bag X17</wicri:noRegion>
</affiliation>
</author>
<author>
<name sortKey="Wilson, C D" sort="Wilson, C D" uniqKey="Wilson C" first="C. D." last="Wilson">C. D. Wilson</name>
<affiliation wicri:level="4">
<inist:fA14 i1="18">
<s1>Department of Physics & Astronomy, McMaster University</s1>
<s2>Hamilton, Ontario L8S 4M1</s2>
<s3>CAN</s3>
<sZ>32 aut.</sZ>
</inist:fA14>
<country>Canada</country>
<placeName>
<settlement type="city">Hamilton (Ontario)</settlement>
<region type="state">Ontario</region>
</placeName>
<orgName type="university">Université McMaster</orgName>
</affiliation>
</author>
<author>
<name sortKey="Waelkens, C" sort="Waelkens, C" uniqKey="Waelkens C" first="C." last="Waelkens">C. Waelkens</name>
<affiliation wicri:level="3">
<inist:fA14 i1="06">
<s1>Instituut voor Sterrenkunde, KU Leuven, Celestijnenlaan 200D</s1>
<s2>3001 Leuven</s2>
<s3>BEL</s3>
<sZ>11 aut.</sZ>
<sZ>33 aut.</sZ>
</inist:fA14>
<country>Belgique</country>
<placeName>
<region type="province" nuts="2">Province du Brabant flamand</region>
<settlement type="town">Heverlee</settlement>
<settlement type="city">Louvain</settlement>
</placeName>
</affiliation>
</author>
</analytic>
<series>
<title level="j" type="main">Astronomy and astrophysics : (Berlin. Print)</title>
<title level="j" type="abbreviated">Astron. astrophys. : (Berl., Print)</title>
<idno type="ISSN">0004-6361</idno>
<imprint>
<date when="2012">2012</date>
</imprint>
</series>
</biblStruct>
</sourceDesc>
<seriesStmt>
<title level="j" type="main">Astronomy and astrophysics : (Berlin. Print)</title>
<title level="j" type="abbreviated">Astron. astrophys. : (Berl., Print)</title>
<idno type="ISSN">0004-6361</idno>
</seriesStmt>
</fileDesc>
<profileDesc>
<textClass>
<keywords scheme="KwdEn" xml:lang="en">
<term>Data reduction</term>
<term>Gas to dust ratio</term>
<term>Metallicity</term>
<term>Morphology</term>
<term>Nearest neighbour</term>
<term>Ring structure</term>
<term>Spiral galaxies</term>
<term>Star formation</term>
</keywords>
<keywords scheme="Pascal" xml:lang="fr">
<term>Galaxies spirales</term>
<term>Morphologie</term>
<term>Plus proche voisin</term>
<term>Formation stellaire</term>
<term>Réduction donnée</term>
<term>Structure annulaire</term>
<term>Rapport gaz poussière</term>
<term>Métallicité</term>
</keywords>
</textClass>
</profileDesc>
</teiHeader>
<front>
<div type="abstract" xml:lang="en">Context. We have obtained Herschel images at five wavelengths from 100 to 500 μm of a ∼5.5 x 2.5 degree area centred on the local galaxy M 31 (Andromeda), our nearest neighbour spiral galaxy, as part of the Herschel guaranteed time project "HELGA". The main goals of HELGA are to study the characteristics of the extended dust emission, focusing on larger scales than studied in previous observations of Andromeda at an increased spatial resolution, and the obscured star formation. Aims. In this paper we present data reduction and Herschel maps, and provide a description of the far-infrared morphology, comparing it with features seen at other wavelengths. Methods. We used high-resolution maps of the atomic hydrogen, fully covering our fields, to identify dust emission features that can be associated to M 31 with confidence, distinguishing them from emission coming from the foreground Galactic cirrus. Results. Thanks to the very large extension of our maps we detect, for the first time at far-infrared wavelengths, three arc-like structures extending out to ∼21, ∼26 and ∼31 kpc respectively, in the south-western part of M 31. The presence of these features, hosting ∼2.2 x 10
<sup>6</sup>
M
<sub>◦.</sub>
of dust, is safely confirmed by their detection in HI maps. Overall, we estimate a total dust mass of ∼5.8 x 10
<sup>7</sup>
M
<sub>◦.</sub>
, about 78% of which is contained in the two main ring-like structures at 10 and 15 kpc, at an average temperature of 16.5 K. We find that the gas-to-dust ratio declines exponentially as a function of the galacto-centric distance, in agreement with the known metallicity gradient, with values ranging from 66 in the nucleus to ∼275 in the outermost region. Conclusions. Dust in M31 extends significantly beyond its optical radius (∼21 kpc) and what was previously mapped in the far-infrared. An annular-like segment, located approximately at R
<sub>25</sub>
, is clearly detected on both sides of the galaxy, and two other similar annular structures are undoubtedly detected on the south-west side even further out.</div>
</front>
</TEI>
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<list>
<country>
<li>Afrique du Sud</li>
<li>Allemagne</li>
<li>Australie</li>
<li>Belgique</li>
<li>Canada</li>
<li>France</li>
<li>Italie</li>
<li>Royaume-Uni</li>
<li>États-Unis</li>
</country>
<region>
<li>Angleterre</li>
<li>Grand Londres</li>
<li>Grand Manchester</li>
<li>Latium</li>
<li>Massachusetts</li>
<li>Ontario</li>
<li>Provence-Alpes-Côte d'Azur</li>
<li>Province de Flandre-Orientale</li>
<li>Province du Brabant flamand</li>
<li>Vienne (Autriche)</li>
<li>Île-de-France</li>
</region>
<settlement>
<li>Amherst (Massachusetts)</li>
<li>Gand</li>
<li>Gif-sur-Yvette</li>
<li>Hamilton (Ontario)</li>
<li>Heverlee</li>
<li>Londres</li>
<li>Louvain</li>
<li>Manchester</li>
<li>Marseille</li>
<li>Paris</li>
<li>Rome</li>
<li>Vienne (Autriche)</li>
</settlement>
<orgName>
<li>University College de Londres</li>
<li>Université McMaster</li>
<li>Université de Gand</li>
<li>Université de Manchester</li>
<li>Université du Massachusetts</li>
</orgName>
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<name sortKey="Fritz, J" sort="Fritz, J" uniqKey="Fritz J" first="J." last="Fritz">J. Fritz</name>
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<name sortKey="Baes, M" sort="Baes, M" uniqKey="Baes M" first="M." last="Baes">M. Baes</name>
<name sortKey="Blommaert, J A D L" sort="Blommaert, J A D L" uniqKey="Blommaert J" first="J. A. D. L." last="Blommaert">J. A. D. L. Blommaert</name>
<name sortKey="De Looze, I" sort="De Looze, I" uniqKey="De Looze I" first="I." last="De Looze">I. De Looze</name>
<name sortKey="Gentile, G" sort="Gentile, G" uniqKey="Gentile G" first="G." last="Gentile">G. Gentile</name>
<name sortKey="Gentile, G" sort="Gentile, G" uniqKey="Gentile G" first="G." last="Gentile">G. Gentile</name>
<name sortKey="Gordon, K D" sort="Gordon, K D" uniqKey="Gordon K" first="K. D." last="Gordon">K. D. Gordon</name>
<name sortKey="Verstappen, J" sort="Verstappen, J" uniqKey="Verstappen J" first="J." last="Verstappen">J. Verstappen</name>
<name sortKey="Waelkens, C" sort="Waelkens, C" uniqKey="Waelkens C" first="C." last="Waelkens">C. Waelkens</name>
</country>
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</noRegion>
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<name sortKey="Eales, S A" sort="Eales, S A" uniqKey="Eales S" first="S. A." last="Eales">S. A. Eales</name>
<name sortKey="Ford, G P" sort="Ford, G P" uniqKey="Ford G" first="G. P." last="Ford">G. P. Ford</name>
<name sortKey="Gear, W K" sort="Gear, W K" uniqKey="Gear W" first="W. K." last="Gear">W. K. Gear</name>
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<name sortKey="Kirk, J" sort="Kirk, J" uniqKey="Kirk J" first="J." last="Kirk">J. Kirk</name>
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</country>
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</noRegion>
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<noRegion>
<name sortKey="Duval, J Roman" sort="Duval, J Roman" uniqKey="Duval J" first="J. Roman" last="Duval">J. Roman Duval</name>
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<name sortKey="Gordon, K D" sort="Gordon, K D" uniqKey="Gordon K" first="K. D." last="Gordon">K. D. Gordon</name>
<name sortKey="Thilker, D" sort="Thilker, D" uniqKey="Thilker D" first="D." last="Thilker">D. Thilker</name>
</country>
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<region name="Provence-Alpes-Côte d'Azur">
<name sortKey="Boquien, M" sort="Boquien, M" uniqKey="Boquien M" first="M." last="Boquien">M. Boquien</name>
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<name sortKey="Boselli, A" sort="Boselli, A" uniqKey="Boselli A" first="A." last="Boselli">A. Boselli</name>
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<name sortKey="Lebouteiller, V" sort="Lebouteiller, V" uniqKey="Lebouteiller V" first="V." last="Lebouteiller">V. Lebouteiller</name>
<name sortKey="Madden, S C" sort="Madden, S C" uniqKey="Madden S" first="S. C." last="Madden">S. C. Madden</name>
<name sortKey="Remy, A" sort="Remy, A" uniqKey="Remy A" first="A." last="Remy">A. Remy</name>
<name sortKey="Roussel, H" sort="Roussel, H" uniqKey="Roussel H" first="H." last="Roussel">H. Roussel</name>
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<noRegion>
<name sortKey="Cortese, L" sort="Cortese, L" uniqKey="Cortese L" first="L." last="Cortese">L. Cortese</name>
</noRegion>
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<region name="Latium">
<name sortKey="Spinoglio, L" sort="Spinoglio, L" uniqKey="Spinoglio L" first="L." last="Spinoglio">L. Spinoglio</name>
</region>
</country>
<country name="Afrique du Sud">
<noRegion>
<name sortKey="Vaccari, M" sort="Vaccari, M" uniqKey="Vaccari M" first="M." last="Vaccari">M. Vaccari</name>
</noRegion>
</country>
<country name="Canada">
<region name="Ontario">
<name sortKey="Wilson, C D" sort="Wilson, C D" uniqKey="Wilson C" first="C. D." last="Wilson">C. D. Wilson</name>
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