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Deep Herschel view of obscured star formation in the Bullet cluster

dc.contributor.authorPérez González, Pablo Guillermo
dc.contributor.authorotros, ...
dc.date.accessioned2023-06-20T04:15:57Z
dc.date.available2023-06-20T04:15:57Z
dc.date.issued2010-07
dc.description© ESO, 2010. Artículo firmado por 36 autores. This work is based in part on observations made with Herschel, a European Space Agency Cornerstone Mission with significant participation by NASA. Support for this work was provided by NASA through an award issued by JPL/Caltech.
dc.description.abstractWe use deep, five band (100–500 μm) data from the Herschel Lensing Survey (HLS) to fully constrain the obscured star formation rate, SFR_FIR, of galaxies in the Bullet cluster (z = 0.296), and a smaller background system (z = 0.35) in the same field. Herschel detects 23 Bullet cluster members with a total SFR_FIR = 144±14 M_⨀ yr^-1. On average, the background system contains brighter far-infrared (FIR) galaxies, with ~50% higher SFR_FIR (21 galaxies; 207± 9 M_⨀ yr^-1). SFRs extrapolated from 24 μm flux via recent templates (SFR_24 µm) agree well with SFRFIR for ~60% of the cluster galaxies. In the remaining ~40%, SFR_24 µm underestimates SFR_FIR due to a significant excess in observed S_100/S_24 (rest frame S_75/S_18) compared to templates of the same FIR luminosity.
dc.description.departmentDepto. de Física de la Tierra y Astrofísica
dc.description.facultyFac. de Ciencias Físicas
dc.description.refereedTRUE
dc.description.sponsorshipNational Aeronautics and Space Administration (NASA)
dc.description.statuspub
dc.eprint.idhttps://eprints.ucm.es/id/eprint/38556
dc.identifier.doi10.1051/0004-6361/201014681
dc.identifier.issn0004-6361
dc.identifier.officialurlhttp://dx.doi.org/10.1051/0004-6361/201014681
dc.identifier.relatedurlhttp://www.aanda.org/
dc.identifier.urihttps://hdl.handle.net/20.500.14352/45107
dc.journal.titleAstronomy & Astrophysics
dc.language.isoeng
dc.publisherEDP Sciencies
dc.rights.accessRightsopen access
dc.subject.cdu52
dc.subject.keywordInfrared galaxies
dc.subject.keyword1E0657-56
dc.subject.keywordFilaments
dc.subject.keywordSpitzer
dc.subject.ucmAstrofísica
dc.subject.ucmAstronomía (Física)
dc.titleDeep Herschel view of obscured star formation in the Bullet cluster
dc.typejournal article
dc.volume.number518
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dspace.entity.typePublication
relation.isAuthorOfPublicationa57c0327-fab0-44e0-9b9c-24b1f7081391
relation.isAuthorOfPublication.latestForDiscoverya57c0327-fab0-44e0-9b9c-24b1f7081391

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