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First 450-micron dust continuum mapping of the massive star-forming region NGC 3576 with the P-ArTeMiS bolometer camera

dc.contributor.authorANDRÉ, P.
hal.structure.identifierDépartement d'Astrophysique, de physique des Particules, de physique Nucléaire et de l'Instrumentation Associée [DAPNIA]
dc.contributor.authorMINIER, V.
dc.contributor.authorGALLAIS, P.
hal.structure.identifierESO
dc.contributor.authorREVERET, V.
dc.contributor.authorPENNEC, J. Le
hal.structure.identifierSolar-Terrestrial Centre of Excellence [Brussels] [STCE]
dc.contributor.authorRODRIGUEZ, L.
hal.structure.identifierDépartement d'Astrophysique, de physique des Particules, de physique Nucléaire et de l'Instrumentation Associée [DAPNIA]
dc.contributor.authorBOULADE, O.
dc.contributor.authorDOUMAYROU, E.
hal.structure.identifierChimie Et Interdisciplinarité : Synthèse, Analyse, Modélisation [CEISAM]
dc.contributor.authorDUBREUIL, D.
dc.contributor.authorLORTHOLARY, M.
dc.contributor.authorMARTIGNAC, J.
hal.structure.identifierAstrophysique Interprétation Modélisation [AIM (UMR7158 / UMR_E_9005 / UM_112)]
dc.contributor.authorTALVARD, M.
hal.structure.identifierInstitut d'Astrophysique de Paris [IAP]
dc.contributor.authorDE BREUCK, C.
dc.contributor.authorHAMON, G.
hal.structure.identifierDepartment of Health Sciences Research [Mayo Clinic] [HSR]
dc.contributor.authorSCHNEIDER, N.
hal.structure.identifierLaboratoire Hétérochimie Fondamentale et Appliquée [LHFA]
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
hal.structure.identifierInstitut de Recherches sur les lois Fondamentales de l'Univers [IRFU]
dc.contributor.authorLAGAGE, P. O.
hal.structure.identifierInstitut de Recherches sur les lois Fondamentales de l'Univers [IRFU]
dc.contributor.authorPANTIN, E.
hal.structure.identifierLaboratoire des matériaux et du génie physique [LMGP ]
dc.contributor.authorROUSSEL, Hervé
hal.structure.identifierChemical Laboratories
dc.contributor.authorMILLER, M.
hal.structure.identifierSwinburne University of Technology (Hawthorn campus)
dc.contributor.authorPURCELL, C. R.
hal.structure.identifierAquatic Environment Research Centre
dc.contributor.authorHILL, T.
dc.contributor.authorSTUTZKI, J.
dc.date.accessioned2021-07-07T16:47:58Z
dc.date.available2021-07-07T16:47:58Z
dc.date.issued2008
dc.identifier.issn0004-6361
dc.identifier.urihttps://oskar-bordeaux.fr/handle/20.500.12278/97413
dc.description.abstractEnContext: The earliest phases of massive star formation are currently much debated. Aims. In an effort to make progress, we took a census of Class0-like protostellar dense cores in the NGC 3576 region, one of the nearest and most luminous embedded sites of high-mass star formation in the Galaxy. Methods: We used the P-ArTeMiS bolometer camera on the APEX telescope to produce the first 450-micron dust continuum map of the filamentary dense clump associated with NGC 3576. Results: Combining our 450-micron observations with existing data at other wavelengths, we have identified seven massive protostellar sources along the NGC 3576 filament and placed them in the M_env - L_bol evolutionary diagram for protostars. Conclusions: Comparison with theoretical evolutionary tracks suggests that these seven protostellar sources will evolve into massive stars with masses M* ~ 15-50 Msun. Four sources are classified as candidate high-mass Class 0 objects, two sources as massive Class I objects, and one source appears to be at an intermediate stage.
dc.language.isoen
dc.publisherEDP Sciences
dc.subject.enstars: formation
dc.subject.enstars: circumstellar matter
dc.subject.enISM: clouds
dc.subject.enISM: structure
dc.subject.enISM: individual objects: NGC 3576
dc.subject.ensubmillimeter
dc.title.enFirst 450-micron dust continuum mapping of the massive star-forming region NGC 3576 with the P-ArTeMiS bolometer camera
dc.typeArticle de revue
dc.identifier.doi10.1051/0004-6361:200810957
dc.subject.halPhysique [physics]/Astrophysique [astro-ph]/Cosmologie et astrophysique extra-galactique [astro-ph.CO]
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]/Planétologie et astrophysique de la terre [astro-ph.EP]
dc.identifier.arxiv0809.3968
bordeaux.journalAstronomy and Astrophysics - A&A
bordeaux.pageL27-L30
bordeaux.volume490
bordeaux.hal.laboratoriesLaboratoire d'Astrophysique de Bordeaux (LAB) - UMR 5804*
bordeaux.issue3
bordeaux.institutionCNRS
bordeaux.institutionUniversité de Bordeaux
bordeaux.peerReviewedoui
hal.identifierhal-00400781
hal.version1
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-00400781v1
bordeaux.COinSctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.jtitle=Astronomy%20and%20Astrophysics%20-%20A&A&rft.date=2008&rft.volume=490&rft.issue=3&rft.spage=L27-L30&rft.epage=L27-L30&rft.eissn=0004-6361&rft.issn=0004-6361&rft.au=ANDR%C3%89,%20P.&MINIER,%20V.&GALLAIS,%20P.&REVERET,%20V.&PENNEC,%20J.%20Le&rft.genre=article


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