hal.structure.identifier | Herzberg Institute of Astrophysics | |
dc.contributor.author | DI FRANCESCO, J. | |
hal.structure.identifier | Herzberg Institute of Astrophysics | |
dc.contributor.author | SADAVOY, S. | |
hal.structure.identifier | Institut de Recherches sur les lois Fondamentales de l'Univers [IRFU] | |
hal.structure.identifier | Astrophysique Interprétation Modélisation [AIM (UMR7158 / UMR_E_9005 / UM_112)] | |
dc.contributor.author | MOTTE, F. | |
hal.structure.identifier | Astrophysique Interprétation Modélisation [AIM (UMR7158 / UMR_E_9005 / UM_112)] | |
dc.contributor.author | SCHNEIDER, N. | |
hal.structure.identifier | Astrophysique Interprétation Modélisation [AIM (UMR7158 / UMR_E_9005 / UM_112)] | |
dc.contributor.author | HENNEMANN, M. | |
hal.structure.identifier | Laboratoire d'Astrophysique de Bordeaux [Pessac] [LAB] | |
hal.structure.identifier | Observatoire aquitain des sciences de l'univers [OASU] | |
hal.structure.identifier | Université Sciences et Technologies - Bordeaux 1 [UB] | |
hal.structure.identifier | Laboratoire d'astrodynamique, d'astrophysique et d'aéronomie de bordeaux [L3AB] | |
dc.contributor.author | BONTEMPS, Sylvain | |
hal.structure.identifier | Astrophysique Interprétation Modélisation [AIM (UMR7158 / UMR_E_9005 / UM_112)] | |
dc.contributor.author | CSENGERI, T. | |
hal.structure.identifier | Max-Planck-Institut für Astronomie [MPIA] | |
dc.contributor.author | BALOG, Z. | |
hal.structure.identifier | Laboratoire d'Astrophysique de Marseille [LAM] | |
hal.structure.identifier | Observatoire Astronomique de Marseille Provence [OAMP] | |
dc.contributor.author | ZAVAGNO, Annie | |
hal.structure.identifier | Astrophysique Interprétation Modélisation [AIM (UMR7158 / UMR_E_9005 / UM_112)] | |
dc.contributor.author | ANDRE, Ph. | |
hal.structure.identifier | Istituto di Fisica dello Spazio Interplanetario [IFSI] | |
dc.contributor.author | SARACENO, P. | |
hal.structure.identifier | School of Physics and Astronomy [Cardiff] | |
dc.contributor.author | GRIFFIN, M. | |
hal.structure.identifier | Astrophysique Interprétation Modélisation [AIM (UMR7158 / UMR_E_9005 / UM_112)] | |
dc.contributor.author | MEN'SHCHIKOV, A. | |
hal.structure.identifier | Institut d'astrophysique spatiale [IAS] | |
dc.contributor.author | ABERGEL, A. | |
hal.structure.identifier | Laboratoire d'Astrophysique de Marseille [LAM] | |
dc.contributor.author | BALUTEAU, J. -P. | |
hal.structure.identifier | Centre d'étude spatiale des rayonnements [CESR] | |
dc.contributor.author | BERNARD, J. -Ph. | |
dc.contributor.author | COX, P. | |
hal.structure.identifier | Laboratoire d'Astrophysique de Marseille [LAM] | |
hal.structure.identifier | Observatoire Astronomique de Marseille Provence [OAMP] | |
dc.contributor.author | DEHARVENG, L. | |
hal.structure.identifier | Astrophysique Interprétation Modélisation [AIM (UMR7158 / UMR_E_9005 / UM_112)] | |
dc.contributor.author | DIDELON, P. | |
dc.contributor.author | DI GIORGIO, A. -M. | |
dc.contributor.author | HARGRAVE, P. | |
hal.structure.identifier | National Astronomical Observatories [Beijing] [NAOC] | |
dc.contributor.author | HUANG, M. | |
hal.structure.identifier | School of Physics and Astronomy [Cardiff] | |
dc.contributor.author | KIRK, J. | |
hal.structure.identifier | STFC Rutherford Appleton Laboratory [RAL] | |
dc.contributor.author | LEEKS, S. | |
hal.structure.identifier | National Astronomical Observatories [Beijing] [NAOC] | |
dc.contributor.author | LI, J. Z. | |
dc.contributor.author | MARSTON, A. | |
hal.structure.identifier | CITA | |
dc.contributor.author | MARTIN, P. | |
hal.structure.identifier | Astrophysique Interprétation Modélisation [AIM (UMR7158 / UMR_E_9005 / UM_112)] | |
hal.structure.identifier | Institut de Recherches sur les lois Fondamentales de l'Univers [IRFU] | |
dc.contributor.author | MINIER, V. | |
hal.structure.identifier | Istituto di Fisica dello Spazio Interplanetario [IFSI] | |
dc.contributor.author | MOLINARI, S. | |
hal.structure.identifier | Stockholm University | |
dc.contributor.author | OLOFSSON, G. | |
hal.structure.identifier | Istituto di Fisica dello Spazio Interplanetario [IFSI] | |
dc.contributor.author | PERSI, P. | |
hal.structure.identifier | Istituto di Fisica dello Spazio Interplanetario [IFSI] | |
dc.contributor.author | PEZZUTO, S. | |
hal.structure.identifier | Laboratoire d'Astrophysique de Marseille [LAM] | |
dc.contributor.author | RUSSEIL, D. | |
hal.structure.identifier | Astrophysique Interprétation Modélisation [AIM (UMR7158 / UMR_E_9005 / UM_112)] | |
dc.contributor.author | SAUVAGE, M. | |
hal.structure.identifier | Royal Observatory Edinburgh [ROE] | |
dc.contributor.author | SIBTHORPE, B. | |
hal.structure.identifier | Antarctic Research a European Network for Astrophysics [ARENA] | |
dc.contributor.author | SPINOGLIO, L. | |
hal.structure.identifier | European Southern Observatory [ESO] | |
dc.contributor.author | TESTI, L. | |
hal.structure.identifier | Herschel Science Center [Madrid] | |
dc.contributor.author | TEYSSIER, D. | |
dc.contributor.author | VAVREK, R. | |
hal.structure.identifier | School of Physics and Astronomy [Cardiff] | |
dc.contributor.author | WARD-THOMPSON, D. | |
hal.structure.identifier | STFC Rutherford Appleton Laboratory [RAL] | |
dc.contributor.author | WHITE, G. | |
hal.structure.identifier | University of Exeter | |
dc.contributor.author | WILSON, C. | |
hal.structure.identifier | Royal Observatory Edinburgh [ROE] | |
dc.contributor.author | WOODCRAFT, A. | |
dc.date.created | 2010 | |
dc.date.issued | 2010 | |
dc.identifier.issn | 0004-6361 | |
dc.description.abstractEn | We present a preliminary analysis of the small-scale structure found in new 70-520 micron continuum maps of the Rosette molecular cloud (RMC), obtained with the SPIRE and PACS instruments of the Herschel Space Observatory. We find 473 clumps within the RMC using a new structure identification algorithm, with sizes up to ~1.0 pc in diameter. A comparison with recent Spitzer maps reveals that 371 clumps are "starless" (without an associated young stellar object), while 102 are "protostellar." Using the respective values of dust temperature, we determine the clumps have masses (M_C) over the range -0.75 <= log (M_C/M_sun) <= 2.50. Linear fits to the high-mass tails of the resulting clump mass spectra (CMS) have slopes that are consistent with those found for high-mass clumps identified in CO emission by other groups. | |
dc.language.iso | en | |
dc.publisher | EDP Sciences | |
dc.title.en | Small-scale structure in the Rosette molecular cloud revealed by Herschel | |
dc.type | Article de revue | |
dc.identifier.doi | 10.1051/0004-6361/201014598 | |
dc.subject.hal | Planète et Univers [physics]/Astrophysique [astro-ph]/Astrophysique stellaire et solaire [astro-ph.SR] | |
dc.subject.hal | Physique [physics]/Astrophysique [astro-ph]/Astrophysique stellaire et solaire [astro-ph.SR] | |
dc.identifier.arxiv | 1005.3784 | |
bordeaux.journal | Astronomy and Astrophysics - A&A | |
bordeaux.page | L91 | |
bordeaux.volume | 518 | |
bordeaux.peerReviewed | oui | |
hal.identifier | hal-00523472 | |
hal.version | 1 | |
hal.popular | non | |
hal.audience | Internationale | |
hal.origin.link | https://hal.archives-ouvertes.fr//hal-00523472v1 | |
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