Deep Herschel view of obscured star formation in the Bullet cluster
dc.contributor.author | Pérez González, Pablo Guillermo | |
dc.contributor.author | otros, ... | |
dc.date.accessioned | 2023-06-20T04:15:57Z | |
dc.date.available | 2023-06-20T04:15:57Z | |
dc.date.issued | 2010-07 | |
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.abstract | We 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.department | Depto. de Física de la Tierra y Astrofísica | |
dc.description.faculty | Fac. de Ciencias Físicas | |
dc.description.refereed | TRUE | |
dc.description.sponsorship | National Aeronautics and Space Administration (NASA) | |
dc.description.status | pub | |
dc.eprint.id | https://eprints.ucm.es/id/eprint/38556 | |
dc.identifier.doi | 10.1051/0004-6361/201014681 | |
dc.identifier.issn | 0004-6361 | |
dc.identifier.officialurl | http://dx.doi.org/10.1051/0004-6361/201014681 | |
dc.identifier.relatedurl | http://www.aanda.org/ | |
dc.identifier.uri | https://hdl.handle.net/20.500.14352/45107 | |
dc.journal.title | Astronomy & Astrophysics | |
dc.language.iso | eng | |
dc.publisher | EDP Sciencies | |
dc.rights.accessRights | open access | |
dc.subject.cdu | 52 | |
dc.subject.keyword | Infrared galaxies | |
dc.subject.keyword | 1E0657-56 | |
dc.subject.keyword | Filaments | |
dc.subject.keyword | Spitzer | |
dc.subject.ucm | Astrofísica | |
dc.subject.ucm | Astronomía (Física) | |
dc.title | Deep Herschel view of obscured star formation in the Bullet cluster | |
dc.type | journal article | |
dc.volume.number | 518 | |
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dspace.entity.type | Publication | |
relation.isAuthorOfPublication | a57c0327-fab0-44e0-9b9c-24b1f7081391 | |
relation.isAuthorOfPublication.latestForDiscovery | a57c0327-fab0-44e0-9b9c-24b1f7081391 |
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