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VizieR Online Data Catalog: M33 molecular clouds and young stellar clusters (Corbelli+, 2017)

dc.contributor.authorCORBELLI, E.
hal.structure.identifierFORMATION STELLAIRE 2017
dc.contributor.authorBRAINE, J.
dc.contributor.authorBANDIERA, R.
hal.structure.identifierFORMATION STELLAIRE 2017
dc.contributor.authorBROUILLET, N.
hal.structure.identifierLaboratoire d'Etude du Rayonnement et de la Matière en Astrophysique [LERMA]
hal.structure.identifierCollège de France - Chaire Galaxies et cosmologie
dc.contributor.authorCOMBES, F.
hal.structure.identifierFORMATION STELLAIRE 2017
dc.contributor.authorDRUARD, C.
hal.structure.identifierAMOR 2017
dc.contributor.authorGRATIER, P.
hal.structure.identifierCentro de Geologia [Lisboa]
dc.contributor.authorMATA, J.
hal.structure.identifierInstitut de RadioAstronomie Millimétrique [IRAM]
dc.contributor.authorSCHUSTER, K.
hal.structure.identifierInstitute for Astronomy, Astrophysics, Space Applications and Remote Sensing [Penteli] [IAASARS]
dc.contributor.authorXILOURIS, M.
hal.structure.identifierMuséum national d'Histoire naturelle [MNHN]
dc.contributor.authorPALLA, F.
dc.date.issued2017-04
dc.descriptionVizieR On-line Data Catalog: J/A+A/601/A146. Originally published in: 2017A&A...601A.146C
dc.description.abstractEnTable 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.isoen
dc.subject.enCarbon monoxide
dc.subject.enMolecular clouds
dc.subject.enInterstellar medium
dc.subject.enGalaxies: nearby
dc.title.enVizieR Online Data Catalog: M33 molecular clouds and young stellar clusters (Corbelli+, 2017)
dc.typeAutre document
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]/Cosmologie et astrophysique extra-galactique [astro-ph.CO]
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]/Astrophysique galactique [astro-ph.GA]
hal.identifierhal-01533168
hal.version1
hal.popularnon
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-01533168v1
bordeaux.COinSctx_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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