100 mum and 160 mum emission as resolved star-formation rate estimators in M33 (HERM33ES)
| hal.structure.identifier | Astrophysique Interprétation Modélisation [AIM (UMR7158 / UMR_E_9005 / UM_112)] | |
| hal.structure.identifier | Department of Astronomy | |
| dc.contributor.author | BOQUIEN, M. | |
| hal.structure.identifier | Department of Astronomy | |
| dc.contributor.author | CALZETTI, D. | |
| hal.structure.identifier | Instituto de RadioAstronomía Milimétrica [IRAM] | |
| dc.contributor.author | KRAMER, C. | |
| dc.contributor.author | XILOURIS, E. M. | |
| hal.structure.identifier | Max-Planck-Institut für Radioastronomie [MPIFR] | |
| dc.contributor.author | BERTOLDI, F. | |
| hal.structure.identifier | Observatoire aquitain des sciences de l'univers [OASU] | |
| hal.structure.identifier | Laboratoire d'Astrophysique de Bordeaux [Pessac] [LAB] | |
| hal.structure.identifier | Université Sciences et Technologies - Bordeaux 1 [UB] | |
| hal.structure.identifier | Laboratoire d'astrodynamique, d'astrophysique et d'aéronomie de bordeaux [L3AB] | |
| dc.contributor.author | BRAINE, J. | |
| hal.structure.identifier | Instituto de RadioAstronomía Milimétrica [IRAM] | |
| dc.contributor.author | BUCHBENDER, C. | |
| hal.structure.identifier | Laboratoire d'Etude du Rayonnement et de la Matière en Astrophysique [LERMA] | |
| dc.contributor.author | COMBES, F. | |
| hal.structure.identifier | Leiden Observatory [Leiden] | |
| dc.contributor.author | ISRAEL, F. | |
| hal.structure.identifier | Australia Telescope National Facility | |
| dc.contributor.author | KORIBALSKI, B. | |
| dc.contributor.author | LORD, S. | |
| hal.structure.identifier | Instituto de RadioAstronomía Milimétrica [IRAM] | |
| dc.contributor.author | QUINTANA-LACACI, G. | |
| hal.structure.identifier | Dpto. Fisica Teorica y del Cosmos | |
| dc.contributor.author | RELAÑO, M. | |
| dc.contributor.author | RÖLLIG, M. | |
| dc.contributor.author | STACEY, G. | |
| dc.contributor.author | TABATABAEI, F. S. | |
| dc.contributor.author | TILANUS, R. P. J. | |
| dc.contributor.author | VAN DER TAK, F. | |
| dc.contributor.author | VAN DER WERF, P. | |
| hal.structure.identifier | Dept. fısica Teorica y del Cosmos | |
| dc.contributor.author | VERLEY, S. | |
| dc.date.created | 2010-05-12 | |
| dc.date.issued | 2010 | |
| dc.identifier.issn | 0004-6361 | |
| dc.description.abstractEn | Over the past few years several studies have provided estimates of the SFR (star-formation rate) or the total infrared luminosity from just one infrared band. However these relations are generally derived for entire galaxies, which are known to contain a large scale diffuse emission that is not necessarily related to the latest star-formation episode. We provide new relations to estimate the SFR from resolved star-forming regions at 100 mum and 160 mum. We select individual star-forming regions in the nearby (840 kpc) galaxy M33. We estimate the SFR combining the emission in Halpha and at 24 mum to calibrate the emission at 100 mum and 160 mum as SFR estimators, as mapped with PACS/Herschel. The data are obtained in the framework of the HERM33ES open time key project. There is less emission in the HII regions at 160 mum than at 100 mum. Over a dynamic range of almost 2 dex in Sigma(SFR) we find that the 100 mum emission is a nearly linear estimator of the SFR, whereas that at 160 mum is slightly superlinear. The behaviour of individual star-forming regions is surprisingly similar to that of entire galaxies. At high Sigma(SFR), star formation drives the dust temperature, whereas uncertainties and variations in radiation-transfer and dust-heated processes dominate at low Sigma(SFR). Detailed modelling of both galaxies and individual star forming regions will be needed to interpret similarities and differences between the two and assess the fraction of diffuse emission in galaxies. | |
| dc.language.iso | en | |
| dc.publisher | EDP Sciences | |
| dc.subject.en | Cosmology and Extragalactic Astrophysics | |
| dc.subject.en | Astrophysics | |
| dc.subject.en | Galaxy Astrophysics | |
| dc.title.en | 100 mum and 160 mum emission as resolved star-formation rate estimators in M33 (HERM33ES) | |
| dc.type | Article de revue | |
| dc.identifier.doi | 10.1051/0004-6361/201014649 | |
| dc.subject.hal | Planète et Univers [physics]/Astrophysique [astro-ph]/Astrophysique stellaire et solaire [astro-ph.SR] | |
| dc.subject.hal | Physique [physics]/Astrophysique [astro-ph]/Astrophysique stellaire et solaire [astro-ph.SR] | |
| dc.identifier.arxiv | 1005.2182 | |
| bordeaux.journal | Astronomy and Astrophysics - A&A | |
| bordeaux.page | L70 | |
| bordeaux.volume | 518 | |
| bordeaux.peerReviewed | oui | |
| hal.identifier | hal-00495883 | |
| hal.version | 1 | |
| hal.popular | non | |
| hal.audience | Internationale | |
| hal.origin.link | https://hal.archives-ouvertes.fr//hal-00495883v1 | |
| bordeaux.COinS | ctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.jtitle=Astronomy%20and%20Astrophysics%20-%20A&A&rft.date=2010&rft.volume=518&rft.spage=L70&rft.epage=L70&rft.eissn=0004-6361&rft.issn=0004-6361&rft.au=BOQUIEN,%20M.&CALZETTI,%20D.&KRAMER,%20C.&XILOURIS,%20E.%20M.&BERTOLDI,%20F.&rft.genre=article |
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