Resolving the Vela C ridge with P-ArTeMiS and Herschel
| hal.structure.identifier | Astrophysique Interprétation Modélisation [AIM (UMR7158 / UMR_E_9005 / UM_112)] | |
| dc.contributor.author | HILL, T. | |
| hal.structure.identifier | Astrophysique Interprétation Modélisation [AIM (UMR7158 / UMR_E_9005 / UM_112)] | |
| dc.contributor.author | ANDRE, Ph. | |
| dc.contributor.author | ARZOUMANIAN, D. | |
| hal.structure.identifier | Institut de Recherches sur les lois Fondamentales de l'Univers [IRFU] | |
| dc.contributor.author | MOTTE, F. | |
| hal.structure.identifier | Institut de Recherches sur les lois Fondamentales de l'Univers [IRFU] | |
| dc.contributor.author | MINIER, V. | |
| dc.contributor.author | MENSHCHIKOV, A. | |
| hal.structure.identifier | Astrophysique Interprétation Modélisation [AIM (UMR7158 / UMR_E_9005 / UM_112)] | |
| dc.contributor.author | DIDELON, P. | |
| hal.structure.identifier | Astrophysique Interprétation Modélisation [AIM (UMR7158 / UMR_E_9005 / UM_112)] | |
| dc.contributor.author | HENNEMANN, M. | |
| dc.contributor.author | KONYVES, V. | |
| hal.structure.identifier | Astrophysique Interprétation Modélisation [AIM (UMR7158 / UMR_E_9005 / UM_112)] | |
| dc.contributor.author | NGUYEN-LUONG, Q. | |
| dc.contributor.author | PALMEIRIM, P. | |
| hal.structure.identifier | Astrophysique Interprétation Modélisation [AIM (UMR7158 / UMR_E_9005 / UM_112)] | |
| dc.contributor.author | PERETTO, N. | |
| hal.structure.identifier | FORMATION STELLAIRE 2012 | |
| dc.contributor.author | SCHNEIDER, N. | |
| hal.structure.identifier | FORMATION STELLAIRE 2012 | |
| dc.contributor.author | BONTEMPS, Sylvain | |
| hal.structure.identifier | Groupe d'Etudes des Matériaux Hétérogènes [GEMH] | |
| dc.contributor.author | LOUVET, François | |
| dc.contributor.author | ELIA, D. | |
| hal.structure.identifier | foreign laboratories [FL] | |
| dc.contributor.author | GIANNINI, T. | |
| dc.contributor.author | REVERET, V. | |
| dc.contributor.author | PENNEC, J. Le | |
| dc.contributor.author | RODRIGUEZ, L. | |
| hal.structure.identifier | Institut de Recherches sur les lois Fondamentales de l'Univers [IRFU] | |
| dc.contributor.author | BOULADE, O. | |
| hal.structure.identifier | Institut de Recherches sur les lois Fondamentales de l'Univers [IRFU] | |
| dc.contributor.author | DOUMAYROU, E. | |
| hal.structure.identifier | Institut de Recherches sur les lois Fondamentales de l'Univers [IRFU] | |
| dc.contributor.author | DUBREUIL, D. | |
| hal.structure.identifier | Institut de Recherches sur les lois Fondamentales de l'Univers [IRFU] | |
| dc.contributor.author | GALLAIS, P. | |
| hal.structure.identifier | Institut de Recherches sur les lois Fondamentales de l'Univers [IRFU] | |
| dc.contributor.author | LORTHOLARY, M. | |
| hal.structure.identifier | Département d'Astrophysique, de physique des Particules, de physique Nucléaire et de l'Instrumentation Associée [DAPNIA] | |
| dc.contributor.author | MARTIGNAC, J. | |
| hal.structure.identifier | Institut de Recherches sur les lois Fondamentales de l'Univers [IRFU] | |
| dc.contributor.author | TALVARD, M. | |
| hal.structure.identifier | Institut d'Astrophysique de Paris [IAP] | |
| dc.contributor.author | DE BREUCK, C. | |
| dc.date.created | 2012-11-01 | |
| dc.date.issued | 2012 | |
| dc.identifier.issn | 0004-6361 | |
| dc.description.abstractEn | We present APEX/P-ArTéMiS 450\mu m continuum observations of RCW 36 and the adjacent ridge, a high-mass high-column density filamentary structure at the centre of the Vela C molecular cloud. These observations, at higher resolution than Herschel's SPIRE camera, reveal clear fragmentation of the central star-forming ridge. Combined with PACS far-infrared and SPIRE sub-millimetre observations from the Herschel HOBYS project we build a high resolution column density map of the region mapped with P-ArTéMiS. We extract the radial density profile of the Vela C ridge which with a ~ 0.1pc central width is consistent with that measured for low-mass star-forming filaments in the Herschel Gould Belt survey. Direct comparison with Serpens South, of the Gould Belt Aquila complex, reveals many similarities between the two regions. Despite likely different formation mechanisms and histories, the Vela C ridge and Serpens South filament share common characteristics, including their filament central widths. | |
| dc.language.iso | en | |
| dc.publisher | EDP Sciences | |
| dc.title.en | Resolving the Vela C ridge with P-ArTeMiS and Herschel | |
| dc.type | Article de revue | |
| dc.identifier.doi | 10.1051/0004-6361/201220504 | |
| dc.subject.hal | Physique [physics]/Astrophysique [astro-ph]/Astrophysique stellaire et solaire [astro-ph.SR] | |
| dc.subject.hal | Planète et Univers [physics]/Astrophysique [astro-ph]/Astrophysique stellaire et solaire [astro-ph.SR] | |
| dc.identifier.arxiv | 1211.0275 | |
| bordeaux.journal | Astronomy and Astrophysics - A&A | |
| bordeaux.page | id.L6 | |
| bordeaux.volume | 548 | |
| bordeaux.peerReviewed | oui | |
| hal.identifier | hal-00838764 | |
| hal.version | 1 | |
| hal.popular | non | |
| hal.audience | Internationale | |
| hal.origin.link | https://hal.archives-ouvertes.fr//hal-00838764v1 | |
| bordeaux.COinS | ctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.jtitle=Astronomy%20and%20Astrophysics%20-%20A&A&rft.date=2012&rft.volume=548&rft.spage=id.L6&rft.epage=id.L6&rft.eissn=0004-6361&rft.issn=0004-6361&rft.au=HILL,%20T.&ANDRE,%20Ph.&ARZOUMANIAN,%20D.&MOTTE,%20F.&MINIER,%20V.&rft.genre=article |
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