Variation in the dust spectral index across M33
dc.contributor.author | TABATABAEI, F. S. | |
hal.structure.identifier | FORMATION STELLAIRE 2011 | |
dc.contributor.author | BRAINE, J. | |
hal.structure.identifier | Instituto de RadioAstronomía Milimétrica [IRAM] | |
dc.contributor.author | KRAMER, C. | |
dc.contributor.author | XILOURIS, M. | |
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 | Dept. fısica Teorica y del Cosmos | |
dc.contributor.author | VERLEY, S. | |
dc.contributor.author | SCHINNERER, E. | |
hal.structure.identifier | Department of Astronomy | |
dc.contributor.author | CALZETTI, D. | |
dc.contributor.author | COMBES, F. | |
hal.structure.identifier | Leiden Observatory [Leiden] | |
dc.contributor.author | ISRAEL, F. | |
hal.structure.identifier | Institut für Physik [Potsdam] | |
dc.contributor.author | HENKEL, C. | |
dc.contributor.author | THE HERM33ES TEAM | |
dc.date.issued | 2011-11 | |
dc.date.conference | 2011 | |
dc.description.abstractEn | Using the Herschel PACS and SPIRE FIR/submm data, we investigate variations in the dust spectral index $\beta$ in the nearby spiral galaxy M33 at a linear resolution of 160 pc. We use an iteration method in two different approaches, single and two-component modified black body models. In both approaches, $\beta$ is higher in the central disk than in the outer disk similar to the dust temperature. There is a positive correlation between $\beta$ and Halpha as well as with the molecular gas traced by CO(2-1). A Monte-Carlo simulation shows that the physical parameters are better constrained when using the two-component model. | |
dc.language.iso | en | |
dc.source.title | Proceedings IAU Symposium No. 284, 2011, R.J. Tuffs & C.C.Popescu, eds | |
dc.subject.en | Astrophysics | |
dc.subject.en | Cosmology and Extragalactic Astrophysics | |
dc.title.en | Variation in the dust spectral index across M33 | |
dc.type | Communication dans un congrès | |
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 | 6740 | |
bordeaux.volume | 1111 | |
bordeaux.conference.title | The Spectral Energy Distribution of Galaxies | |
bordeaux.country | GB | |
bordeaux.title.proceeding | Proceedings IAU Symposium No. 284, 2011, R.J. Tuffs & C.C.Popescu, eds | |
bordeaux.conference.city | Preston | |
bordeaux.peerReviewed | oui | |
hal.identifier | hal-00650920 | |
hal.version | 1 | |
hal.invited | non | |
hal.proceedings | oui | |
hal.popular | non | |
hal.audience | Internationale | |
hal.origin.link | https://hal.archives-ouvertes.fr//hal-00650920v1 | |
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