Molecular gas in the halo fuels the growth of a massive cluster galaxy at high redshift.
Identifieur interne : 001A44 ( PubMed/Checkpoint ); précédent : 001A43; suivant : 001A45Molecular gas in the halo fuels the growth of a massive cluster galaxy at high redshift.
Auteurs : B H C. Emonts [Espagne] ; M D Lehnert [France] ; M. Villar-Martín [Espagne] ; R P Norris [Australie] ; R D Ekers [Australie] ; G A Van Moorsel [États-Unis] ; H. Dannerbauer [Espagne] ; L. Pentericci [Italie] ; G K Miley [Pays-Bas] ; J R Allison [Australie] ; E M Sadler [Australie] ; P. Guillard [France] ; C L Carilli [États-Unis] ; M Y Mao [Pays-Bas] ; H J A. Röttgering [Pays-Bas] ; C. De Breuck [Allemagne] ; N. Seymour [Australie] ; B. Gullberg [Royaume-Uni] ; D. Ceverino [Espagne] ; P. Jagannathan [États-Unis] ; J. Vernet [Allemagne] ; B T Indermuehle [Australie]Source :
- Science (New York, N.Y.) [ 1095-9203 ] ; 2016.
Abstract
The largest galaxies in the universe reside in galaxy clusters. Using sensitive observations of carbon monoxide, we show that the Spiderweb galaxy-a massive galaxy in a distant protocluster-is forming from a large reservoir of molecular gas. Most of this molecular gas lies between the protocluster galaxies and has low velocity dispersion, indicating that it is part of an enriched intergalactic medium. This may constitute the reservoir of gas that fuels the widespread star formation seen in earlier ultraviolet observations of the Spiderweb galaxy. Our results support the notion that giant galaxies in clusters formed from extended regions of recycled gas at high redshift.
DOI: 10.1126/science.aag0512
PubMed: 27934760
Affiliations:
- Allemagne, Australie, Espagne, France, Italie, Pays-Bas, Royaume-Uni, États-Unis
- Communauté de Madrid, Nouveau-Mexique, Nouvelle-Galles du Sud, Île-de-France
- Madrid, Paris, Sydney
- Université de Sydney
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pubmed:27934760Le document en format XML
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<author><name sortKey="Carilli, C L" sort="Carilli, C L" uniqKey="Carilli C" first="C L" last="Carilli">C L Carilli</name>
<affiliation wicri:level="2"><nlm:affiliation>National Radio Astronomy Observatory, Socorro, NM 87801, USA.</nlm:affiliation>
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<wicri:regionArea>National Radio Astronomy Observatory, Socorro, NM 87801</wicri:regionArea>
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<author><name sortKey="Mao, M Y" sort="Mao, M Y" uniqKey="Mao M" first="M Y" last="Mao">M Y Mao</name>
<affiliation wicri:level="1"><nlm:affiliation>Joint Institute for Very Long Baseline Interferometry, European Research Infrastructure Consortium, 7990 AA Dwingeloo, Netherlands.</nlm:affiliation>
<country xml:lang="fr">Pays-Bas</country>
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<author><name sortKey="Rottgering, H J A" sort="Rottgering, H J A" uniqKey="Rottgering H" first="H J A" last="Röttgering">H J A. Röttgering</name>
<affiliation wicri:level="1"><nlm:affiliation>Leiden Observatory, University of Leiden, 2300 RA Leiden, Netherlands.</nlm:affiliation>
<country xml:lang="fr">Pays-Bas</country>
<wicri:regionArea>Leiden Observatory, University of Leiden, 2300 RA Leiden</wicri:regionArea>
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<affiliation wicri:level="1"><nlm:affiliation>European Southern Observatory, 85748 Garching, Germany.</nlm:affiliation>
<country xml:lang="fr">Allemagne</country>
<wicri:regionArea>European Southern Observatory, 85748 Garching</wicri:regionArea>
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<wicri:regionArea>International Centre for Radio Astronomy Research, Curtin University, Perth</wicri:regionArea>
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<author><name sortKey="Gullberg, B" sort="Gullberg, B" uniqKey="Gullberg B" first="B" last="Gullberg">B. Gullberg</name>
<affiliation wicri:level="1"><nlm:affiliation>Centre for Extragalactic Astronomy, Department of Physics, Durham University, Durham DH1 3LE, UK.</nlm:affiliation>
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<wicri:noRegion>Durham DH1 3LE</wicri:noRegion>
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<author><name sortKey="Ceverino, D" sort="Ceverino, D" uniqKey="Ceverino D" first="D" last="Ceverino">D. Ceverino</name>
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<region nuts="2" type="region">Communauté de Madrid</region>
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</author>
<author><name sortKey="Jagannathan, P" sort="Jagannathan, P" uniqKey="Jagannathan P" first="P" last="Jagannathan">P. Jagannathan</name>
<affiliation wicri:level="2"><nlm:affiliation>National Radio Astronomy Observatory, Socorro, NM 87801, USA.</nlm:affiliation>
<country xml:lang="fr">États-Unis</country>
<wicri:regionArea>National Radio Astronomy Observatory, Socorro, NM 87801</wicri:regionArea>
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<author><name sortKey="Vernet, J" sort="Vernet, J" uniqKey="Vernet J" first="J" last="Vernet">J. Vernet</name>
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<country xml:lang="fr">Allemagne</country>
<wicri:regionArea>European Southern Observatory, 85748 Garching</wicri:regionArea>
<wicri:noRegion>85748 Garching</wicri:noRegion>
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<wicri:noRegion>85748 Garching</wicri:noRegion>
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<author><name sortKey="Indermuehle, B T" sort="Indermuehle, B T" uniqKey="Indermuehle B" first="B T" last="Indermuehle">B T Indermuehle</name>
<affiliation wicri:level="1"><nlm:affiliation>Commonwealth Scientific and Industrial Research Organisation, Astronomy and Space Science, Australia Telescope National Facility, Epping, NSW 1710, Australia.</nlm:affiliation>
<country xml:lang="fr">Australie</country>
<wicri:regionArea>Commonwealth Scientific and Industrial Research Organisation, Astronomy and Space Science, Australia Telescope National Facility, Epping, NSW 1710</wicri:regionArea>
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<series><title level="j">Science (New York, N.Y.)</title>
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<imprint><date when="2016" type="published">2016</date>
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<front><div type="abstract" xml:lang="en">The largest galaxies in the universe reside in galaxy clusters. Using sensitive observations of carbon monoxide, we show that the Spiderweb galaxy-a massive galaxy in a distant protocluster-is forming from a large reservoir of molecular gas. Most of this molecular gas lies between the protocluster galaxies and has low velocity dispersion, indicating that it is part of an enriched intergalactic medium. This may constitute the reservoir of gas that fuels the widespread star formation seen in earlier ultraviolet observations of the Spiderweb galaxy. Our results support the notion that giant galaxies in clusters formed from extended regions of recycled gas at high redshift.</div>
</front>
</TEI>
<pubmed><MedlineCitation Status="PubMed-not-MEDLINE" Owner="NLM"><PMID Version="1">27934760</PMID>
<DateCreated><Year>2016</Year>
<Month>12</Month>
<Day>09</Day>
</DateCreated>
<DateCompleted><Year>2017</Year>
<Month>07</Month>
<Day>31</Day>
</DateCompleted>
<DateRevised><Year>2017</Year>
<Month>07</Month>
<Day>31</Day>
</DateRevised>
<Article PubModel="Print"><Journal><ISSN IssnType="Electronic">1095-9203</ISSN>
<JournalIssue CitedMedium="Internet"><Volume>354</Volume>
<Issue>6316</Issue>
<PubDate><Year>2016</Year>
<Month>12</Month>
<Day>02</Day>
</PubDate>
</JournalIssue>
<Title>Science (New York, N.Y.)</Title>
<ISOAbbreviation>Science</ISOAbbreviation>
</Journal>
<ArticleTitle>Molecular gas in the halo fuels the growth of a massive cluster galaxy at high redshift.</ArticleTitle>
<Pagination><MedlinePgn>1128-1130</MedlinePgn>
</Pagination>
<Abstract><AbstractText>The largest galaxies in the universe reside in galaxy clusters. Using sensitive observations of carbon monoxide, we show that the Spiderweb galaxy-a massive galaxy in a distant protocluster-is forming from a large reservoir of molecular gas. Most of this molecular gas lies between the protocluster galaxies and has low velocity dispersion, indicating that it is part of an enriched intergalactic medium. This may constitute the reservoir of gas that fuels the widespread star formation seen in earlier ultraviolet observations of the Spiderweb galaxy. Our results support the notion that giant galaxies in clusters formed from extended regions of recycled gas at high redshift.</AbstractText>
<CopyrightInformation>Copyright © 2016, American Association for the Advancement of Science.</CopyrightInformation>
</Abstract>
<AuthorList CompleteYN="Y"><Author ValidYN="Y"><LastName>Emonts</LastName>
<ForeName>B H C</ForeName>
<Initials>BH</Initials>
<AffiliationInfo><Affiliation>Centro de Astrobiología (Consejo Superior de Investigaciones Científicas-Instituto Nacional de Técnica Aerospacial), Carretera de Torrejón a Ajalvir, km 4, 28850 Torrejón de Ardoz, Madrid, Spain. bjornemonts@gmail.com.</Affiliation>
</AffiliationInfo>
</Author>
<Author ValidYN="Y"><LastName>Lehnert</LastName>
<ForeName>M D</ForeName>
<Initials>MD</Initials>
<AffiliationInfo><Affiliation>Sorbonne Universités, Université Pierre et Marie Curie, Université Paris 6 et Centre National de la Recherche Scientifique, Unité Mixte de Recherche 7095, Institut d'Astrophysique de Paris, 75014 Paris, France.</Affiliation>
</AffiliationInfo>
</Author>
<Author ValidYN="Y"><LastName>Villar-Martín</LastName>
<ForeName>M</ForeName>
<Initials>M</Initials>
<AffiliationInfo><Affiliation>Centro de Astrobiología (Consejo Superior de Investigaciones Científicas-Instituto Nacional de Técnica Aerospacial), Carretera de Torrejón a Ajalvir, km 4, 28850 Torrejón de Ardoz, Madrid, Spain.</Affiliation>
</AffiliationInfo>
<AffiliationInfo><Affiliation>Facultad de Ciencias, Unidad Asociada Consejo Superior de Investigaciones Científicas, Astro-Universidad Autónoma de Madrid, Campus de Cantoblanco, 28049 Madrid, Spain.</Affiliation>
</AffiliationInfo>
</Author>
<Author ValidYN="Y"><LastName>Norris</LastName>
<ForeName>R P</ForeName>
<Initials>RP</Initials>
<AffiliationInfo><Affiliation>Commonwealth Scientific and Industrial Research Organisation, Astronomy and Space Science, Australia Telescope National Facility, Epping, NSW 1710, Australia.</Affiliation>
</AffiliationInfo>
<AffiliationInfo><Affiliation>Western Sydney University, Penrith South, NSW 1797, Australia.</Affiliation>
</AffiliationInfo>
</Author>
<Author ValidYN="Y"><LastName>Ekers</LastName>
<ForeName>R D</ForeName>
<Initials>RD</Initials>
<AffiliationInfo><Affiliation>Commonwealth Scientific and Industrial Research Organisation, Astronomy and Space Science, Australia Telescope National Facility, Epping, NSW 1710, Australia.</Affiliation>
</AffiliationInfo>
</Author>
<Author ValidYN="Y"><LastName>van Moorsel</LastName>
<ForeName>G A</ForeName>
<Initials>GA</Initials>
<AffiliationInfo><Affiliation>National Radio Astronomy Observatory, Socorro, NM 87801, USA.</Affiliation>
</AffiliationInfo>
</Author>
<Author ValidYN="Y"><LastName>Dannerbauer</LastName>
<ForeName>H</ForeName>
<Initials>H</Initials>
<AffiliationInfo><Affiliation>Instituto de Astrofísica de Canarias, E-38205 La Laguna, Tenerife, Spain.</Affiliation>
</AffiliationInfo>
<AffiliationInfo><Affiliation>Departamento Astrofísica, Universidad de La Laguna, E-38206 La Laguna, Tenerife, Spain.</Affiliation>
</AffiliationInfo>
<AffiliationInfo><Affiliation>Institut für Astrophysik, Universität Wien, 1180 Wien, Austria.</Affiliation>
</AffiliationInfo>
</Author>
<Author ValidYN="Y"><LastName>Pentericci</LastName>
<ForeName>L</ForeName>
<Initials>L</Initials>
<AffiliationInfo><Affiliation>Istituto Nazionale di Astrofisica, Osservatorio Astronomico di Roma, 00040 Monteporzio (RM), Italy.</Affiliation>
</AffiliationInfo>
</Author>
<Author ValidYN="Y"><LastName>Miley</LastName>
<ForeName>G K</ForeName>
<Initials>GK</Initials>
<AffiliationInfo><Affiliation>Leiden Observatory, University of Leiden, 2300 RA Leiden, Netherlands.</Affiliation>
</AffiliationInfo>
</Author>
<Author ValidYN="Y"><LastName>Allison</LastName>
<ForeName>J R</ForeName>
<Initials>JR</Initials>
<AffiliationInfo><Affiliation>Commonwealth Scientific and Industrial Research Organisation, Astronomy and Space Science, Australia Telescope National Facility, Epping, NSW 1710, Australia.</Affiliation>
</AffiliationInfo>
</Author>
<Author ValidYN="Y"><LastName>Sadler</LastName>
<ForeName>E M</ForeName>
<Initials>EM</Initials>
<AffiliationInfo><Affiliation>Sydney Institute for Astronomy, School of Physics, University of Sydney, NSW 2006, Australia.</Affiliation>
</AffiliationInfo>
</Author>
<Author ValidYN="Y"><LastName>Guillard</LastName>
<ForeName>P</ForeName>
<Initials>P</Initials>
<AffiliationInfo><Affiliation>Sorbonne Universités, Université Pierre et Marie Curie, Université Paris 6 et Centre National de la Recherche Scientifique, Unité Mixte de Recherche 7095, Institut d'Astrophysique de Paris, 75014 Paris, France.</Affiliation>
</AffiliationInfo>
</Author>
<Author ValidYN="Y"><LastName>Carilli</LastName>
<ForeName>C L</ForeName>
<Initials>CL</Initials>
<AffiliationInfo><Affiliation>National Radio Astronomy Observatory, Socorro, NM 87801, USA.</Affiliation>
</AffiliationInfo>
<AffiliationInfo><Affiliation>Cavendish Laboratory, Cambridge CB3 0HE, UK.</Affiliation>
</AffiliationInfo>
</Author>
<Author ValidYN="Y"><LastName>Mao</LastName>
<ForeName>M Y</ForeName>
<Initials>MY</Initials>
<AffiliationInfo><Affiliation>Joint Institute for Very Long Baseline Interferometry, European Research Infrastructure Consortium, 7990 AA Dwingeloo, Netherlands.</Affiliation>
</AffiliationInfo>
<AffiliationInfo><Affiliation>Jodrell Bank Observatory, University of Manchester, Macclesfield, Cheshire SK11 9DL, UK.</Affiliation>
</AffiliationInfo>
</Author>
<Author ValidYN="Y"><LastName>Röttgering</LastName>
<ForeName>H J A</ForeName>
<Initials>HJ</Initials>
<AffiliationInfo><Affiliation>Leiden Observatory, University of Leiden, 2300 RA Leiden, Netherlands.</Affiliation>
</AffiliationInfo>
</Author>
<Author ValidYN="Y"><LastName>De Breuck</LastName>
<ForeName>C</ForeName>
<Initials>C</Initials>
<AffiliationInfo><Affiliation>European Southern Observatory, 85748 Garching, Germany.</Affiliation>
</AffiliationInfo>
</Author>
<Author ValidYN="Y"><LastName>Seymour</LastName>
<ForeName>N</ForeName>
<Initials>N</Initials>
<AffiliationInfo><Affiliation>International Centre for Radio Astronomy Research, Curtin University, Perth, Australia.</Affiliation>
</AffiliationInfo>
</Author>
<Author ValidYN="Y"><LastName>Gullberg</LastName>
<ForeName>B</ForeName>
<Initials>B</Initials>
<AffiliationInfo><Affiliation>Centre for Extragalactic Astronomy, Department of Physics, Durham University, Durham DH1 3LE, UK.</Affiliation>
</AffiliationInfo>
</Author>
<Author ValidYN="Y"><LastName>Ceverino</LastName>
<ForeName>D</ForeName>
<Initials>D</Initials>
<AffiliationInfo><Affiliation>Centro de Astrobiología (Consejo Superior de Investigaciones Científicas-Instituto Nacional de Técnica Aerospacial), Carretera de Torrejón a Ajalvir, km 4, 28850 Torrejón de Ardoz, Madrid, Spain.</Affiliation>
</AffiliationInfo>
<AffiliationInfo><Affiliation>Institut für Theoretische Astrophysik, Zentrum für Astronomie der Universität Heidelberg, 69120 Heidelberg, Germany.</Affiliation>
</AffiliationInfo>
</Author>
<Author ValidYN="Y"><LastName>Jagannathan</LastName>
<ForeName>P</ForeName>
<Initials>P</Initials>
<AffiliationInfo><Affiliation>National Radio Astronomy Observatory, Socorro, NM 87801, USA.</Affiliation>
</AffiliationInfo>
</Author>
<Author ValidYN="Y"><LastName>Vernet</LastName>
<ForeName>J</ForeName>
<Initials>J</Initials>
<AffiliationInfo><Affiliation>European Southern Observatory, 85748 Garching, Germany.</Affiliation>
</AffiliationInfo>
</Author>
<Author ValidYN="Y"><LastName>Indermuehle</LastName>
<ForeName>B T</ForeName>
<Initials>BT</Initials>
<AffiliationInfo><Affiliation>Commonwealth Scientific and Industrial Research Organisation, Astronomy and Space Science, Australia Telescope National Facility, Epping, NSW 1710, Australia.</Affiliation>
</AffiliationInfo>
</Author>
</AuthorList>
<Language>eng</Language>
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<PublicationType UI="D013485">Research Support, Non-U.S. Gov't</PublicationType>
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<Month>05</Month>
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<Month>10</Month>
<Day>21</Day>
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<li>Australie</li>
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<country name="France"><region name="Île-de-France"><name sortKey="Lehnert, M D" sort="Lehnert, M D" uniqKey="Lehnert M" first="M D" last="Lehnert">M D Lehnert</name>
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<name sortKey="Indermuehle, B T" sort="Indermuehle, B T" uniqKey="Indermuehle B" first="B T" last="Indermuehle">B T Indermuehle</name>
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</country>
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</country>
<country name="Royaume-Uni"><noRegion><name sortKey="Gullberg, B" sort="Gullberg, B" uniqKey="Gullberg B" first="B" last="Gullberg">B. Gullberg</name>
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