AustralieFrV1, Main, Exploration, bibRecord, 006B85

Distance determination for RAVE stars using stellar models: III. The nature of the RAVE survey and Milky Way chemistry

Identifieur interne : 006B85 ( Main/Exploration ); précédent : 006B84; suivant : 006B86

Distance determination for RAVE stars using stellar models: III. The nature of the RAVE survey and Milky Way chemistry

Auteurs : B. Burnett [Royaume-Uni] ; J. Binney [Royaume-Uni] ; S. Sharma [Australie] ; M. Williams [Allemagne] ; T. Zwitter [Slovénie] ; O. Bienayme [France] ; J. Bland-Hawthorn [Australie] ; K. C. Freeman [Australie] ; J. Fulbright [États-Unis] ; B. Gibson [Royaume-Uni] ; G. Gilmore [Royaume-Uni] ; E. K. Grebel [Allemagne] ; A. Helmi [Pays-Bas] ; U. Munari [Italie] ; J. F. Navarro [Canada] ; Q. A. Parker [Australie] ; G. M. Seabroke [Royaume-Uni] ; A. Siebert [France] ; A. Siviero [Allemagne, Italie] ; M. Steinmetz [Allemagne] ; F. G. Watson [Australie] ; R. F. G. Wyse [États-Unis]

Source :

Astronomy and astrophysics : (Berlin. Print) [ 0004-6361 ] ; 2011.

RBID : Pascal:11-0486083

Descripteurs français

Pascal (Inist)
- Mesure distance, Modèle stellaire, Voie lactée, Paramètre physique, Catalogue astronomique, Vitesse radiale, Centre galactique, Métallicité, Age, Plan galactique, Galaxies disques, Abondance, Contenu stellaire, Structure galaxies.

English descriptors

KwdEn :
- Abundance, Age, Astronomical catalogues, Disk galaxies, Distance measurement, Galactic centers, Galactic planes, Galaxy structure, Metallicity, Milky Way, Physical parameter, Radial velocity, Star models, Stellar content.

Abstract

We apply the method of Burnett & Binney (2010, MNRAS, 407, 339) for the determination of stellar distances and parameters to the internal catalogue of the RAdial Velocity Experiment (RAVE; Steinmetz et al. 2006, AJ, 132, 1645). Subsamples of stars that either have Hipparcos parallaxes or belong to well-studied clusters inspire confidence in the formal errors. Distances to dwarfs cooler than ∼ 6000 K appear to be unbiased, but those to hotter dwarfs tend to be too small by ∼10% of the formal errors. Distances to giants tend to be too large by about the same amount. The median distance error in the whole sample of 216000 stars is 28% and the error distribution is similar for both giants and dwarfs. Roughly half the stars in the RAVE survey are giants. The giant fraction is largest at low latitudes and in directions towards the Galactic Centre. Near the plane the metallicity distribution is remarkably narrow and centred on [M/H] = -0.04 dex; with increasing |z| it broadens out and its median moves to [M/H] ≃ -0.5. Mean age as a function of distance from the Galactic centre and distance |z| from the Galactic plane shows the anticipated increase in mean age with |z|.

Affiliations:

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Le document en format XML

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<s3>FRA</s3>
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<settlement type="city">Strasbourg</settlement>
</placeName>
<orgName type="university">Université de Strasbourg</orgName>
</affiliation>
</author>
<author><name sortKey="Bland Hawthorn, J" sort="Bland Hawthorn, J" uniqKey="Bland Hawthorn J" first="J." last="Bland-Hawthorn">J. Bland-Hawthorn</name>
<affiliation wicri:level="4"><inist:fA14 i1="02"><s1>Sydney Institute for Astronomy, School of Physics A28, University of Sydney</s1>
<s2>NSW 2006</s2>
<s3>AUS</s3>
<sZ>3 aut.</sZ>
<sZ>7 aut.</sZ>
</inist:fA14>
<country>Australie</country>
<placeName><settlement type="city">Sydney</settlement>
<region type="état">Nouvelle-Galles du Sud</region>
</placeName>
<orgName type="university">Université de Sydney</orgName>
</affiliation>
</author>
<author><name sortKey="Freeman, K C" sort="Freeman, K C" uniqKey="Freeman K" first="K. C." last="Freeman">K. C. Freeman</name>
<affiliation wicri:level="1"><inist:fA14 i1="07"><s1>Research School of Astronomy and Astrophysics, Australian National University, Cotter Rd</s1>
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<s3>AUS</s3>
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</inist:fA14>
<country>Australie</country>
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<author><name sortKey="Fulbright, J" sort="Fulbright, J" uniqKey="Fulbright J" first="J." last="Fulbright">J. Fulbright</name>
<affiliation wicri:level="1"><inist:fA14 i1="08"><s1>Johns Hopkins University, Departement of Physics and Astronomy, 366 Bloomberg center, 3400 N. Charles St</s1>
<s2>Baltimore, MD 21218</s2>
<s3>USA</s3>
<sZ>9 aut.</sZ>
<sZ>22 aut.</sZ>
</inist:fA14>
<country>États-Unis</country>
<wicri:noRegion>Baltimore, MD 21218</wicri:noRegion>
</affiliation>
</author>
<author><name sortKey="Gibson, B" sort="Gibson, B" uniqKey="Gibson B" first="B." last="Gibson">B. Gibson</name>
<affiliation wicri:level="1"><inist:fA14 i1="09"><s1>Jeremiah Horrocks Institute, University of Central Lancashire</s1>
<s2>Preston, PR1 2HE</s2>
<s3>GBR</s3>
<sZ>10 aut.</sZ>
</inist:fA14>
<country>Royaume-Uni</country>
<wicri:noRegion>Preston, PR1 2HE</wicri:noRegion>
</affiliation>
</author>
<author><name sortKey="Gilmore, G" sort="Gilmore, G" uniqKey="Gilmore G" first="G." last="Gilmore">G. Gilmore</name>
<affiliation wicri:level="4"><inist:fA14 i1="10"><s1>Institute of Astronomy, University of Cambridge, Madingley Road</s1>
<s2>Cambridge, CB3 OHA</s2>
<s3>GBR</s3>
<sZ>11 aut.</sZ>
</inist:fA14>
<country>Royaume-Uni</country>
<wicri:noRegion>Cambridge, CB3 OHA</wicri:noRegion>
<orgName type="university">Université de Cambridge</orgName>
<placeName><settlement type="city">Cambridge</settlement>
<region type="country">Angleterre</region>
<region type="région" nuts="1">Angleterre de l'Est</region>
</placeName>
</affiliation>
</author>
<author><name sortKey="Grebel, E K" sort="Grebel, E K" uniqKey="Grebel E" first="E. K." last="Grebel">E. K. Grebel</name>
<affiliation wicri:level="3"><inist:fA14 i1="11"><s1>Astronomisches Rechen-Institut, Zentrum fur Astronomie der Universität Heidelberg, Mönchhofstr. 12-14</s1>
<s2>69120 Heidelberg</s2>
<s3>DEU</s3>
<sZ>12 aut.</sZ>
</inist:fA14>
<country>Allemagne</country>
<placeName><region type="land" nuts="1">Bade-Wurtemberg</region>
<region type="district" nuts="2">District de Karlsruhe</region>
<settlement type="city">Heidelberg</settlement>
</placeName>
</affiliation>
</author>
<author><name sortKey="Helmi, A" sort="Helmi, A" uniqKey="Helmi A" first="A." last="Helmi">A. Helmi</name>
<affiliation wicri:level="4"><inist:fA14 i1="12"><s1>Kapteyn Astronomical Institut, University of Groningen, Landleven 12</s1>
<s2>9747 AD, Groningen</s2>
<s3>NLD</s3>
<sZ>13 aut.</sZ>
</inist:fA14>
<country>Pays-Bas</country>
<placeName><settlement type="city">Groningue</settlement>
<region nuts="2" type="province">Groningue (province)</region>
<settlement type="city">Groningue (ville)</settlement>
</placeName>
<orgName type="university">Université de Groningue</orgName>
</affiliation>
</author>
<author><name sortKey="Munari, U" sort="Munari, U" uniqKey="Munari U" first="U." last="Munari">U. Munari</name>
<affiliation wicri:level="1"><inist:fA14 i1="13"><s1>INAF Osservatorio Astronomico di Padova</s1>
<s2>36012 Asiago (VI</s2>
<s3>ITA</s3>
<sZ>14 aut.</sZ>
</inist:fA14>
<country>Italie</country>
<wicri:noRegion>INAF Osservatorio Astronomico di Padova</wicri:noRegion>
</affiliation>
</author>
<author><name sortKey="Navarro, J F" sort="Navarro, J F" uniqKey="Navarro J" first="J. F." last="Navarro">J. F. Navarro</name>
<affiliation wicri:level="1"><inist:fA14 i1="14"><s1>Department of Physics and Astronomy, University of Victoria, PO Box 3055</s1>
<s2>Victoria, BC V8W 3P6</s2>
<s3>CAN</s3>
<sZ>15 aut.</sZ>
</inist:fA14>
<country>Canada</country>
<wicri:noRegion>Victoria, BC V8W 3P6</wicri:noRegion>
</affiliation>
</author>
<author><name sortKey="Parker, Q A" sort="Parker, Q A" uniqKey="Parker Q" first="Q. A." last="Parker">Q. A. Parker</name>
<affiliation wicri:level="3"><inist:fA14 i1="15"><s1>Department of Physics and Astronomy, Faculty of Sciences, Macquarie University</s1>
<s2>NSW 2109, Sydney</s2>
<s3>AUS</s3>
<sZ>16 aut.</sZ>
</inist:fA14>
<country>Australie</country>
<placeName><settlement type="city">Sydney</settlement>
<region type="état">Nouvelle-Galles du Sud</region>
</placeName>
</affiliation>
</author>
<author><name sortKey="Seabroke, G M" sort="Seabroke, G M" uniqKey="Seabroke G" first="G. M." last="Seabroke">G. M. Seabroke</name>
<affiliation wicri:level="4"><inist:fA14 i1="16"><s1>Mullard Space Science Laboratory, University College London, Holmbury St Mary</s1>
<s2>Dorking, RH5 6NT</s2>
<s3>GBR</s3>
<sZ>17 aut.</sZ>
</inist:fA14>
<country>Royaume-Uni</country>
<wicri:noRegion>Dorking, RH5 6NT</wicri:noRegion>
<orgName type="university">University College de Londres</orgName>
<placeName><settlement type="city">Londres</settlement>
<region type="country">Angleterre</region>
<region type="région" nuts="1">Grand Londres</region>
</placeName>
</affiliation>
</author>
<author><name sortKey="Siebert, A" sort="Siebert, A" uniqKey="Siebert A" first="A." last="Siebert">A. Siebert</name>
<affiliation wicri:level="4"><inist:fA14 i1="06"><s1>Observatoire astronomique de Strasbourg, Universite de Strasbourg, CNRS, UMR 7550, 11 rue de l'université</s1>
<s2>67000 Strasbourg</s2>
<s3>FRA</s3>
<sZ>6 aut.</sZ>
<sZ>18 aut.</sZ>
</inist:fA14>
<country>France</country>
<placeName><region type="region" nuts="2">Grand Est</region>
<region type="old region" nuts="2">Alsace (région administrative)</region>
<settlement type="city">Strasbourg</settlement>
<settlement type="city">Strasbourg</settlement>
</placeName>
<orgName type="university">Université de Strasbourg</orgName>
</affiliation>
</author>
<author><name sortKey="Siviero, A" sort="Siviero, A" uniqKey="Siviero A" first="A." last="Siviero">A. Siviero</name>
<affiliation wicri:level="1"><inist:fA14 i1="03"><s1>Astrophysikalisches Institut Potsdam, An der Sternwarte 16</s1>
<s2>14482 Potsdam</s2>
<s3>DEU</s3>
<sZ>4 aut.</sZ>
<sZ>19 aut.</sZ>
<sZ>20 aut.</sZ>
</inist:fA14>
<country>Allemagne</country>
<wicri:noRegion>14482 Potsdam</wicri:noRegion>
<wicri:noRegion>An der Sternwarte 16</wicri:noRegion>
<wicri:noRegion>14482 Potsdam</wicri:noRegion>
</affiliation>
<affiliation wicri:level="4"><inist:fA14 i1="17"><s1>Dipartimento di Astronomia, Universita di Padova, Vicolo dellŠOsservatorio 2</s1>
<s2>35122 Padova</s2>
<s3>ITA</s3>
<sZ>19 aut.</sZ>
</inist:fA14>
<country>Italie</country>
<wicri:noRegion>35122 Padova</wicri:noRegion>
<orgName type="university">Université de Padoue</orgName>
<placeName><settlement type="city">Padoue</settlement>
<region type="region" nuts="2">Vénétie</region>
</placeName>
</affiliation>
</author>
<author><name sortKey="Steinmetz, M" sort="Steinmetz, M" uniqKey="Steinmetz M" first="M." last="Steinmetz">M. Steinmetz</name>
<affiliation wicri:level="1"><inist:fA14 i1="03"><s1>Astrophysikalisches Institut Potsdam, An der Sternwarte 16</s1>
<s2>14482 Potsdam</s2>
<s3>DEU</s3>
<sZ>4 aut.</sZ>
<sZ>19 aut.</sZ>
<sZ>20 aut.</sZ>
</inist:fA14>
<country>Allemagne</country>
<wicri:noRegion>14482 Potsdam</wicri:noRegion>
<wicri:noRegion>An der Sternwarte 16</wicri:noRegion>
<wicri:noRegion>14482 Potsdam</wicri:noRegion>
</affiliation>
</author>
<author><name sortKey="Watson, F G" sort="Watson, F G" uniqKey="Watson F" first="F. G." last="Watson">F. G. Watson</name>
<affiliation wicri:level="1"><inist:fA14 i1="18"><s1>Australian Astronomical Observatory, PO Box 296</s1>
<s2>Epping, NSW 1710</s2>
<s3>AUS</s3>
<sZ>21 aut.</sZ>
</inist:fA14>
<country>Australie</country>
<wicri:noRegion>Epping, NSW 1710</wicri:noRegion>
</affiliation>
</author>
<author><name sortKey="Wyse, R F G" sort="Wyse, R F G" uniqKey="Wyse R" first="R. F. G." last="Wyse">R. F. G. Wyse</name>
<affiliation wicri:level="1"><inist:fA14 i1="08"><s1>Johns Hopkins University, Departement of Physics and Astronomy, 366 Bloomberg center, 3400 N. Charles St</s1>
<s2>Baltimore, MD 21218</s2>
<s3>USA</s3>
<sZ>9 aut.</sZ>
<sZ>22 aut.</sZ>
</inist:fA14>
<country>États-Unis</country>
<wicri:noRegion>Baltimore, MD 21218</wicri:noRegion>
</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="2011">2011</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>Abundance</term>
<term>Age</term>
<term>Astronomical catalogues</term>
<term>Disk galaxies</term>
<term>Distance measurement</term>
<term>Galactic centers</term>
<term>Galactic planes</term>
<term>Galaxy structure</term>
<term>Metallicity</term>
<term>Milky Way</term>
<term>Physical parameter</term>
<term>Radial velocity</term>
<term>Star models</term>
<term>Stellar content</term>
</keywords>
<keywords scheme="Pascal" xml:lang="fr"><term>Mesure distance</term>
<term>Modèle stellaire</term>
<term>Voie lactée</term>
<term>Paramètre physique</term>
<term>Catalogue astronomique</term>
<term>Vitesse radiale</term>
<term>Centre galactique</term>
<term>Métallicité</term>
<term>Age</term>
<term>Plan galactique</term>
<term>Galaxies disques</term>
<term>Abondance</term>
<term>Contenu stellaire</term>
<term>Structure galaxies</term>
</keywords>
</textClass>
</profileDesc>
</teiHeader>
<front><div type="abstract" xml:lang="en">We apply the method of Burnett & Binney (2010, MNRAS, 407, 339) for the determination of stellar distances and parameters to the internal catalogue of the RAdial Velocity Experiment (RAVE; Steinmetz et al. 2006, AJ, 132, 1645). Subsamples of stars that either have Hipparcos parallaxes or belong to well-studied clusters inspire confidence in the formal errors. Distances to dwarfs cooler than ∼ 6000 K appear to be unbiased, but those to hotter dwarfs tend to be too small by ∼10% of the formal errors. Distances to giants tend to be too large by about the same amount. The median distance error in the whole sample of 216000 stars is 28% and the error distribution is similar for both giants and dwarfs. Roughly half the stars in the RAVE survey are giants. The giant fraction is largest at low latitudes and in directions towards the Galactic Centre. Near the plane the metallicity distribution is remarkably narrow and centred on [M/H] = -0.04 dex; with increasing |z| it broadens out and its median moves to [M/H] ≃ -0.5. Mean age as a function of distance from the Galactic centre and distance |z| from the Galactic plane shows the anticipated increase in mean age with |z|.</div>
</front>
</TEI>
<affiliations><list><country><li>Allemagne</li>
<li>Australie</li>
<li>Canada</li>
<li>France</li>
<li>Italie</li>
<li>Pays-Bas</li>
<li>Royaume-Uni</li>
<li>Slovénie</li>
<li>États-Unis</li>
</country>
<region><li>Alsace (région administrative)</li>
<li>Angleterre</li>
<li>Angleterre de l'Est</li>
<li>Bade-Wurtemberg</li>
<li>District de Karlsruhe</li>
<li>Grand Est</li>
<li>Grand Londres</li>
<li>Groningue (province)</li>
<li>Nouvelle-Galles du Sud</li>
<li>Vénétie</li>
</region>
<settlement><li>Cambridge</li>
<li>Groningue</li>
<li>Groningue (ville)</li>
<li>Heidelberg</li>
<li>Londres</li>
<li>Padoue</li>
<li>Strasbourg</li>
<li>Sydney</li>
</settlement>
<orgName><li>University College de Londres</li>
<li>Université de Cambridge</li>
<li>Université de Groningue</li>
<li>Université de Padoue</li>
<li>Université de Strasbourg</li>
<li>Université de Sydney</li>
</orgName>
</list>
<tree><country name="Royaume-Uni"><noRegion><name sortKey="Burnett, B" sort="Burnett, B" uniqKey="Burnett B" first="B." last="Burnett">B. Burnett</name>
</noRegion>
<name sortKey="Binney, J" sort="Binney, J" uniqKey="Binney J" first="J." last="Binney">J. Binney</name>
<name sortKey="Gibson, B" sort="Gibson, B" uniqKey="Gibson B" first="B." last="Gibson">B. Gibson</name>
<name sortKey="Gilmore, G" sort="Gilmore, G" uniqKey="Gilmore G" first="G." last="Gilmore">G. Gilmore</name>
<name sortKey="Seabroke, G M" sort="Seabroke, G M" uniqKey="Seabroke G" first="G. M." last="Seabroke">G. M. Seabroke</name>
</country>
<country name="Australie"><region name="Nouvelle-Galles du Sud"><name sortKey="Sharma, S" sort="Sharma, S" uniqKey="Sharma S" first="S." last="Sharma">S. Sharma</name>
</region>
<name sortKey="Bland Hawthorn, J" sort="Bland Hawthorn, J" uniqKey="Bland Hawthorn J" first="J." last="Bland-Hawthorn">J. Bland-Hawthorn</name>
<name sortKey="Freeman, K C" sort="Freeman, K C" uniqKey="Freeman K" first="K. C." last="Freeman">K. C. Freeman</name>
<name sortKey="Parker, Q A" sort="Parker, Q A" uniqKey="Parker Q" first="Q. A." last="Parker">Q. A. Parker</name>
<name sortKey="Watson, F G" sort="Watson, F G" uniqKey="Watson F" first="F. G." last="Watson">F. G. Watson</name>
</country>
<country name="Allemagne"><noRegion><name sortKey="Williams, M" sort="Williams, M" uniqKey="Williams M" first="M." last="Williams">M. Williams</name>
</noRegion>
<name sortKey="Grebel, E K" sort="Grebel, E K" uniqKey="Grebel E" first="E. K." last="Grebel">E. K. Grebel</name>
<name sortKey="Siviero, A" sort="Siviero, A" uniqKey="Siviero A" first="A." last="Siviero">A. Siviero</name>
<name sortKey="Steinmetz, M" sort="Steinmetz, M" uniqKey="Steinmetz M" first="M." last="Steinmetz">M. Steinmetz</name>
</country>
<country name="Slovénie"><noRegion><name sortKey="Zwitter, T" sort="Zwitter, T" uniqKey="Zwitter T" first="T." last="Zwitter">T. Zwitter</name>
</noRegion>
<name sortKey="Zwitter, T" sort="Zwitter, T" uniqKey="Zwitter T" first="T." last="Zwitter">T. Zwitter</name>
</country>
<country name="France"><region name="Grand Est"><name sortKey="Bienayme, O" sort="Bienayme, O" uniqKey="Bienayme O" first="O." last="Bienayme">O. Bienayme</name>
</region>
<name sortKey="Siebert, A" sort="Siebert, A" uniqKey="Siebert A" first="A." last="Siebert">A. Siebert</name>
</country>
<country name="États-Unis"><noRegion><name sortKey="Fulbright, J" sort="Fulbright, J" uniqKey="Fulbright J" first="J." last="Fulbright">J. Fulbright</name>
</noRegion>
<name sortKey="Wyse, R F G" sort="Wyse, R F G" uniqKey="Wyse R" first="R. F. G." last="Wyse">R. F. G. Wyse</name>
</country>
<country name="Pays-Bas"><region name="Groningue (province)"><name sortKey="Helmi, A" sort="Helmi, A" uniqKey="Helmi A" first="A." last="Helmi">A. Helmi</name>
</region>
</country>
<country name="Italie"><noRegion><name sortKey="Munari, U" sort="Munari, U" uniqKey="Munari U" first="U." last="Munari">U. Munari</name>
</noRegion>
<name sortKey="Siviero, A" sort="Siviero, A" uniqKey="Siviero A" first="A." last="Siviero">A. Siviero</name>
</country>
<country name="Canada"><noRegion><name sortKey="Navarro, J F" sort="Navarro, J F" uniqKey="Navarro J" first="J. F." last="Navarro">J. F. Navarro</name>
</noRegion>
</country>
</tree>
</affiliations>
</record>

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Distance determination for RAVE stars using stellar models: III. The nature of the RAVE survey and Milky Way chemistry

Distance determination for RAVE stars using stellar models: III. The nature of the RAVE survey and Milky Way chemistry

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