AustralieFrV1, Main, Exploration, bibRecord, 007820

Herschel photometry of brightest cluster galaxies in cooling flow clusters

Identifieur interne : 007820 ( Main/Exploration ); précédent : 007819; suivant : 007821

Herschel photometry of brightest cluster galaxies in cooling flow clusters

Auteurs : A. C. Edge [Royaume-Uni] ; J. B. R. Oonk [Pays-Bas] ; R. Mittal [États-Unis] ; S. W. Allen [États-Unis] ; S. A. Baum [États-Unis] ; H. Böhringer [Allemagne] ; J. N. Bregman [États-Unis] ; M. N. Bremer [Royaume-Uni] ; F. Combes [France] ; C. S. Crawford [Royaume-Uni] ; M. Donahue [États-Unis] ; E. Egami [États-Unis] ; A. C. Fabian [Royaume-Uni] ; G. J. Ferland [États-Unis] ; S. L. Hamer [Royaume-Uni] ; N. A. Hatch [Royaume-Uni] ; W. Jaffe [Pays-Bas] ; R. M. Johnstone [Royaume-Uni] ; B. R. Mcnamara [Canada] ; C. P. O'Dea [États-Unis] ; P. Popesso [Allemagne] ; A. C. Quillen [États-Unis] ; P. Salome [France] ; C. L. Sarazin [États-Unis] ; G. M. Voit [États-Unis] ; R. J. Wilman [Australie] ; M. W. Wise [Pays-Bas]

Source :

Astronomy and astrophysics : (Berlin. Print) [ 0004-6361 ] ; 2010.

RBID : Pascal:11-0086168

Descripteurs français

Pascal (Inist)
- Photométrie, Amas galaxies, Ecoulement refroidissement, Densité élevée, Gaz froid, Rapport gaz poussière, Matière intraamas, Galaxies elliptiques.

English descriptors

KwdEn :
- Cold gas, Cooling flow, Elliptical galaxies, Galaxy clusters, Gas to dust ratio, High density, Intracluster matter, Photometry.

Abstract

The dust destruction timescales in the cores of clusters of galaxies are relatively short given their high central gas densities. However, substantial mid-infrared and sub-mm emission has been detected in many brightest cluster galaxies. In this letter we present Herschel PACS and SPIRE photometry of the brightest cluster galaxy in three strong cooling flow clusters, A1068, A2597 and Zw3146. This photometry indicates that a substantial mass of cold dust is present (>3 x 10⁷ M_◦.) at temperatures significantly lower (20-28 K) than previously thought based on limited MIR and/or sub-mm results. The mass and temperature of the dust appear to match those of the cold gas traced by CO with a gas-to-dust ratio of 80-120.

Affiliations:

Links toward previous steps (curation, corpus...)

to stream PascalFrancis, to step Corpus: 002033
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to stream PascalFrancis, to step Checkpoint: 002360
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Le document en format XML

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<sourceDesc><biblStruct><analytic><title xml:lang="en" level="a">Herschel photometry of brightest cluster galaxies in cooling flow clusters</title>
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<author><name sortKey="Popesso, P" sort="Popesso, P" uniqKey="Popesso P" first="P." last="Popesso">P. Popesso</name>
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<country>Allemagne</country>
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<author><name sortKey="Quillen, A C" sort="Quillen, A C" uniqKey="Quillen A" first="A. C." last="Quillen">A. C. Quillen</name>
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<author><name sortKey="Salome, P" sort="Salome, P" uniqKey="Salome P" first="P." last="Salome">P. Salome</name>
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<author><name sortKey="Sarazin, C L" sort="Sarazin, C L" uniqKey="Sarazin C" first="C. L." last="Sarazin">C. L. Sarazin</name>
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<author><name sortKey="Wilman, R J" sort="Wilman, R J" uniqKey="Wilman R" first="R. J." last="Wilman">R. J. Wilman</name>
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<orgName type="university">Université de Melbourne</orgName>
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</author>
<author><name sortKey="Wise, M W" sort="Wise, M W" uniqKey="Wise M" first="M. W." last="Wise">M. W. Wise</name>
<affiliation wicri:level="1"><inist:fA14 i1="19"><s1>ASTRON, Netherlands Institute for Radio Astronomy, PO Box 2</s1>
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</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="2010">2010</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>Cold gas</term>
<term>Cooling flow</term>
<term>Elliptical galaxies</term>
<term>Galaxy clusters</term>
<term>Gas to dust ratio</term>
<term>High density</term>
<term>Intracluster matter</term>
<term>Photometry</term>
</keywords>
<keywords scheme="Pascal" xml:lang="fr"><term>Photométrie</term>
<term>Amas galaxies</term>
<term>Ecoulement refroidissement</term>
<term>Densité élevée</term>
<term>Gaz froid</term>
<term>Rapport gaz poussière</term>
<term>Matière intraamas</term>
<term>Galaxies elliptiques</term>
</keywords>
</textClass>
</profileDesc>
</teiHeader>
<front><div type="abstract" xml:lang="en">The dust destruction timescales in the cores of clusters of galaxies are relatively short given their high central gas densities. However, substantial mid-infrared and sub-mm emission has been detected in many brightest cluster galaxies. In this letter we present Herschel PACS and SPIRE photometry of the brightest cluster galaxy in three strong cooling flow clusters, A1068, A2597 and Zw3146. This photometry indicates that a substantial mass of cold dust is present (>3 x 10<sup>7</sup>
 M<sub>◦.</sub>
) at temperatures significantly lower (20-28 K) than previously thought based on limited MIR and/or sub-mm results. The mass and temperature of the dust appear to match those of the cold gas traced by CO with a gas-to-dust ratio of 80-120.</div>
</front>
</TEI>
<affiliations><list><country><li>Allemagne</li>
<li>Australie</li>
<li>Canada</li>
<li>France</li>
<li>Pays-Bas</li>
<li>Royaume-Uni</li>
<li>États-Unis</li>
</country>
<region><li>Angleterre</li>
<li>Michigan</li>
<li>Nottinghamshire</li>
<li>Victoria (État)</li>
<li>Île-de-France</li>
</region>
<settlement><li>East Lansing</li>
<li>Melbourne</li>
<li>Nottingham</li>
<li>Paris</li>
</settlement>
<orgName><li>Université d'État du Michigan</li>
<li>Université de Melbourne</li>
<li>Université de Nottingham</li>
</orgName>
</list>
<tree><country name="Royaume-Uni"><noRegion><name sortKey="Edge, A C" sort="Edge, A C" uniqKey="Edge A" first="A. C." last="Edge">A. C. Edge</name>
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<name sortKey="Fabian, A C" sort="Fabian, A C" uniqKey="Fabian A" first="A. C." last="Fabian">A. C. Fabian</name>
<name sortKey="Hamer, S L" sort="Hamer, S L" uniqKey="Hamer S" first="S. L." last="Hamer">S. L. Hamer</name>
<name sortKey="Hatch, N A" sort="Hatch, N A" uniqKey="Hatch N" first="N. A." last="Hatch">N. A. Hatch</name>
<name sortKey="Johnstone, R M" sort="Johnstone, R M" uniqKey="Johnstone R" first="R. M." last="Johnstone">R. M. Johnstone</name>
</country>
<country name="Pays-Bas"><noRegion><name sortKey="Oonk, J B R" sort="Oonk, J B R" uniqKey="Oonk J" first="J. B. R." last="Oonk">J. B. R. Oonk</name>
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<name sortKey="Jaffe, W" sort="Jaffe, W" uniqKey="Jaffe W" first="W." last="Jaffe">W. Jaffe</name>
<name sortKey="Wise, M W" sort="Wise, M W" uniqKey="Wise M" first="M. W." last="Wise">M. W. Wise</name>
</country>
<country name="États-Unis"><noRegion><name sortKey="Mittal, R" sort="Mittal, R" uniqKey="Mittal R" first="R." last="Mittal">R. Mittal</name>
</noRegion>
<name sortKey="Allen, S W" sort="Allen, S W" uniqKey="Allen S" first="S. W." last="Allen">S. W. Allen</name>
<name sortKey="Baum, S A" sort="Baum, S A" uniqKey="Baum S" first="S. A." last="Baum">S. A. Baum</name>
<name sortKey="Bregman, J N" sort="Bregman, J N" uniqKey="Bregman J" first="J. N." last="Bregman">J. N. Bregman</name>
<name sortKey="Donahue, M" sort="Donahue, M" uniqKey="Donahue M" first="M." last="Donahue">M. Donahue</name>
<name sortKey="Egami, E" sort="Egami, E" uniqKey="Egami E" first="E." last="Egami">E. Egami</name>
<name sortKey="Ferland, G J" sort="Ferland, G J" uniqKey="Ferland G" first="G. J." last="Ferland">G. J. Ferland</name>
<name sortKey="O Dea, C P" sort="O Dea, C P" uniqKey="O Dea C" first="C. P." last="O'Dea">C. P. O'Dea</name>
<name sortKey="Quillen, A C" sort="Quillen, A C" uniqKey="Quillen A" first="A. C." last="Quillen">A. C. Quillen</name>
<name sortKey="Sarazin, C L" sort="Sarazin, C L" uniqKey="Sarazin C" first="C. L." last="Sarazin">C. L. Sarazin</name>
<name sortKey="Voit, G M" sort="Voit, G M" uniqKey="Voit G" first="G. M." last="Voit">G. M. Voit</name>
</country>
<country name="Allemagne"><noRegion><name sortKey="Bohringer, H" sort="Bohringer, H" uniqKey="Bohringer H" first="H." last="Böhringer">H. Böhringer</name>
</noRegion>
<name sortKey="Popesso, P" sort="Popesso, P" uniqKey="Popesso P" first="P." last="Popesso">P. Popesso</name>
</country>
<country name="France"><region name="Île-de-France"><name sortKey="Combes, F" sort="Combes, F" uniqKey="Combes F" first="F." last="Combes">F. Combes</name>
</region>
<name sortKey="Salome, P" sort="Salome, P" uniqKey="Salome P" first="P." last="Salome">P. Salome</name>
</country>
<country name="Canada"><noRegion><name sortKey="Mcnamara, B R" sort="Mcnamara, B R" uniqKey="Mcnamara B" first="B. R." last="Mcnamara">B. R. Mcnamara</name>
</noRegion>
</country>
<country name="Australie"><region name="Victoria (État)"><name sortKey="Wilman, R J" sort="Wilman, R J" uniqKey="Wilman R" first="R. J." last="Wilman">R. J. Wilman</name>
</region>
</country>
</tree>
</affiliations>
</record>

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Herschel photometry of brightest cluster galaxies in cooling flow clusters

Herschel photometry of brightest cluster galaxies in cooling flow clusters

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