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Millimeter continuum mapping of Cygnus X (Motte+, 2007)

dc.contributor.authorMOTTE, F.
hal.structure.identifierObservatoire aquitain des sciences de l'univers [OASU]
hal.structure.identifierLaboratoire d'astrodynamique, d'astrophysique et d'aéronomie de bordeaux [L3AB]
hal.structure.identifierLaboratoire d'Astrophysique de Bordeaux [Pessac] [LAB]
dc.contributor.authorBONTEMPS, Sylvain
dc.contributor.authorSCHILKE, P.
dc.contributor.authorSCHNEIDER, N.
dc.contributor.authorK. M., Menten
dc.contributor.authorBROGUIERE, D.
dc.date.issued2007
dc.descriptionVizieR On-line Data Catalog: J/A+A/476/1243. Originally published in: 2007A&A...476.1243M 2007yCat..34761243M
dc.description.abstractEnWe report on a millimeter continuum survey of the entire Cygnus X molecular complex. We used the MAMBO and MAMBO-2 bolometer arrays on the IRAM 30m telescope to map a 3deg2 area at 1.2mm (see fits files of Figures 2, kept to 11" resolution). Our MAMBO-2 imaging gives a complete view of the cloud structures ranging from 0.03pc to 5pc, i.e. from dense cores to clumps. We perform a multi-resolution analysis to extract 129 compact dense cores (~0.1pc, see Table 1) and identify 40 massive large-scale clumps (~0.7pc, see Table 2). The 21um fluxes arising from dense cores are taken from the MSX point source catalog (MSX C6, Cat. ).
dc.language.isoen
dc.title.enMillimeter continuum mapping of Cygnus X (Motte+, 2007)
dc.typeAutre document
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]/Planétologie et astrophysique de la terre [astro-ph.EP]
dc.subject.halPhysique [physics]/Astrophysique [astro-ph]/Planétologie et astrophysique de la terre [astro-ph.EP]
hal.identifierhal-00400791
hal.version1
hal.popularnon
hal.audienceNon spécifiée
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-00400791v1
bordeaux.COinSctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.date=2007&rft.au=MOTTE,%20F.&BONTEMPS,%20Sylvain&SCHILKE,%20P.&SCHNEIDER,%20N.&K.%20M.,%20Menten&rft.genre=unknown


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