M33 HII regions SED (Relano+, 2013)
hal.structure.identifier | Dpto. Fisica Teorica y del Cosmos | |
dc.contributor.author | RELANO, M. | |
hal.structure.identifier | Dept. fısica Teorica y del Cosmos | |
dc.contributor.author | VERLEY, S. | |
dc.contributor.author | PEREZ, I. | |
hal.structure.identifier | Instituto de RadioAstronomía Milimétrica [IRAM] | |
dc.contributor.author | KRAMER, C. | |
hal.structure.identifier | Department of Astronomy | |
dc.contributor.author | CALZETTI, D. | |
dc.contributor.author | XILOURIS, E. M. | |
hal.structure.identifier | Astrophysique Interprétation Modélisation [AIM (UMR7158 / UMR_E_9005 / UM_112)] | |
dc.contributor.author | BOQUIEN, M. | |
dc.contributor.author | ABREU-VICENTE, J. | |
dc.contributor.author | COMBES, F. | |
hal.structure.identifier | Leiden Observatory [Leiden] | |
dc.contributor.author | ISRAEL, F. | |
dc.contributor.author | TABATABAEI, F. S. | |
hal.structure.identifier | FORMATION STELLAIRE 2013 | |
dc.contributor.author | BRAINE, J. | |
hal.structure.identifier | Instituto de RadioAstronomía Milimétrica [IRAM] | |
dc.contributor.author | BUCHBENDER, C. | |
hal.structure.identifier | Astrophysique Interprétation Modélisation [AIM (UMR7158 / UMR_E_9005 / UM_112)] | |
dc.contributor.author | GONZALEZ, M. | |
hal.structure.identifier | Institut de RadioAstronomie Millimétrique [IRAM] | |
dc.contributor.author | GRATIER, P. | |
hal.structure.identifier | Institut de Planétologie et d'Astrophysique de Grenoble [IPAG] | |
dc.contributor.author | LORD, S. | |
hal.structure.identifier | KOSMA, I. Physikalisches Institut | |
dc.contributor.author | MOOKERJEA, B. | |
hal.structure.identifier | Instituto de RadioAstronomía Milimétrica [IRAM] | |
dc.contributor.author | QUINTANA-LACACI, G. | |
hal.structure.identifier | Leiden Observatory [Leiden] | |
dc.contributor.author | VAN DER WERF, P. | |
dc.date.issued | 2013-09 | |
dc.description | VizieR On-line Data Catalog: J/A+A/552/A140. Originally published in: 2013A&A...552A.140R | |
dc.description.abstractEn | To investigate the continuum UV emission of M 33, we used the data from GALEX, in particular the data distributed by de Paz et al. (2007, Cat. J/ApJS/173/185). To trace the ionised gas, we used the narrow-line Hα image of M 33 obtained by Greenawalt (1998, Ph.D. Thesis, New Mexico state University). Dust emission can be investigated through the mid-IR (MIR) and FIR data of M 33 obtained with the Spitzer Infrared Array Camera (IRAC) and Multiband Imaging Photometer (MIPS). (3 data files). | |
dc.language.iso | en | |
dc.subject.en | Galaxies: nearby | |
dc.subject.en | Energy distributions | |
dc.subject.en | Photometry: infrared | |
dc.subject.en | Photometry: ultraviolet | |
dc.title.en | M33 HII regions SED (Relano+, 2013) | |
dc.type | Autre document | |
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] | |
bordeaux.page | 29140 | |
hal.identifier | hal-00880557 | |
hal.version | 1 | |
hal.popular | non | |
hal.audience | Non spécifiée | |
hal.origin.link | https://hal.archives-ouvertes.fr//hal-00880557v1 | |
bordeaux.COinS | ctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.date=2013-09&rft.spage=29140&rft.epage=29140&rft.au=RELANO,%20M.&VERLEY,%20S.&PEREZ,%20I.&KRAMER,%20C.&CALZETTI,%20D.&rft.genre=unknown |
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