VizieR Online Data Catalog: M33 molecular clouds and young stellar clusters (Corbelli+, 2017)
dc.contributor.author | CORBELLI, E. | |
hal.structure.identifier | FORMATION STELLAIRE 2017 | |
dc.contributor.author | BRAINE, J. | |
dc.contributor.author | BANDIERA, R. | |
hal.structure.identifier | FORMATION STELLAIRE 2017 | |
dc.contributor.author | BROUILLET, N. | |
hal.structure.identifier | Laboratoire d'Etude du Rayonnement et de la Matière en Astrophysique [LERMA] | |
hal.structure.identifier | Collège de France - Chaire Galaxies et cosmologie | |
dc.contributor.author | COMBES, F. | |
hal.structure.identifier | FORMATION STELLAIRE 2017 | |
dc.contributor.author | DRUARD, C. | |
hal.structure.identifier | AMOR 2017 | |
dc.contributor.author | GRATIER, P. | |
hal.structure.identifier | Centro de Geologia [Lisboa] | |
dc.contributor.author | MATA, J. | |
hal.structure.identifier | Institut de RadioAstronomie Millimétrique [IRAM] | |
dc.contributor.author | SCHUSTER, K. | |
hal.structure.identifier | Institute for Astronomy, Astrophysics, Space Applications and Remote Sensing [Penteli] [IAASARS] | |
dc.contributor.author | XILOURIS, M. | |
hal.structure.identifier | Muséum national d'Histoire naturelle [MNHN] | |
dc.contributor.author | PALLA, F. | |
dc.date.issued | 2017-04 | |
dc.description | VizieR On-line Data Catalog: J/A+A/601/A146. Originally published in: 2017A&A...601A.146C | |
dc.description.abstractEn | Table 5 : Physical parameters for the 566 molecular clouds identified through the IRAM 30m CO J=2-1 survey of the star forming disk of M33. For each cloud the cloud type and the following properties are listed: celestial coordinates, galactocentric radius, cloud deconvolved effective radius and its uncertainty, CO(2-1) line velocity dispersion from CPROPS and its uncertainty, line velocity dispersion from a Gaussian fit, CO luminous mass and its uncertainty, and virial mass from a Gaussian fit. In the last column the identification number of the young stellar cluster candidates associated with the molecular cloud are listed. Notes: We identify up to four young stellar cluster candidates (YSCCs) associated with each molecular cloud and we list them according to the identification number of Sharma et al. (2011, Cat. J/A+A/545/A96) given also in Table 6. Table 6 : Physical parameters for the 630 young stellar cluster candidates identified via their mid-infrared emission in the star forming disk of M33. For each YSCC we list the type of source, the identified number of the molecular clouds associated with it (if any) and the corresponding cloud classes. In addition, for each YSCC we give the celestial coordinates, the bolometric, total infrared, FUV and Halpha luminosities, the estimated mass and age, the visual extinction, the galactocentric radius, the source size, and its flux at 24μm. (2 data files). | |
dc.language.iso | en | |
dc.subject.en | Carbon monoxide | |
dc.subject.en | Molecular clouds | |
dc.subject.en | Interstellar medium | |
dc.subject.en | Galaxies: nearby | |
dc.title.en | VizieR Online Data Catalog: M33 molecular clouds and young stellar clusters (Corbelli+, 2017) | |
dc.type | Autre document | |
dc.subject.hal | Planète et Univers [physics]/Astrophysique [astro-ph]/Cosmologie et astrophysique extra-galactique [astro-ph.CO] | |
dc.subject.hal | Planète et Univers [physics]/Astrophysique [astro-ph]/Astrophysique galactique [astro-ph.GA] | |
hal.identifier | hal-01533168 | |
hal.version | 1 | |
hal.popular | non | |
hal.origin.link | https://hal.archives-ouvertes.fr//hal-01533168v1 | |
bordeaux.COinS | ctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.date=2017-04&rft.au=CORBELLI,%20E.&BRAINE,%20J.&BANDIERA,%20R.&BROUILLET,%20N.&COMBES,%20F.&rft.genre=unknown |
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