Initial highlights of the Herschel imaging survey of OB Young Stellar objects (HOBYS)
MOTTE, F.
Astrophysique Interprétation Modélisation [AIM (UMR7158 / UMR_E_9005 / UM_112)]
Institut de Recherches sur les lois Fondamentales de l'Univers [IRFU]
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Astrophysique Interprétation Modélisation [AIM (UMR7158 / UMR_E_9005 / UM_112)]
Institut de Recherches sur les lois Fondamentales de l'Univers [IRFU]
MOTTE, F.
Astrophysique Interprétation Modélisation [AIM (UMR7158 / UMR_E_9005 / UM_112)]
Institut de Recherches sur les lois Fondamentales de l'Univers [IRFU]
Astrophysique Interprétation Modélisation [AIM (UMR7158 / UMR_E_9005 / UM_112)]
Institut de Recherches sur les lois Fondamentales de l'Univers [IRFU]
ZAVAGNO, Annie
Laboratoire d'Astrophysique de Marseille [LAM]
Observatoire Astronomique de Marseille Provence [OAMP]
< Reduce
Laboratoire d'Astrophysique de Marseille [LAM]
Observatoire Astronomique de Marseille Provence [OAMP]
Language
en
Communication dans un congrès
This item was published in
SF2A-2010, SF2A-2010, SF2A-2010: Proceedings of the Annual meeting of the French Society of Astronomy and Astrophysics. Eds.: S. Boissier, M. Heydari-Malayeri, R. Samadi and D. Valls-Gabaud - 21 - 24 June 2010, Marseille, p.225, 2010, 2010, Marseille. 2010-12p. 225
English Abstract
We present initial Herschel HOBYS highlights of the Rosette molecular complex. The five Herschel wavebands of SPIRE (250/350/500~μm) and PACS (70 and 160~μm) allows HOBYS to provide an unbiased and complete census of ...Read more >
We present initial Herschel HOBYS highlights of the Rosette molecular complex. The five Herschel wavebands of SPIRE (250/350/500~μm) and PACS (70 and 160~μm) allows HOBYS to provide an unbiased and complete census of intermediate- to high-mass young stellar objects, some of which are not detected by Spitzer. Key core properties, derived from spectral energy distributions, such as bolometric luminosity and mass, are used to constrain their evolutionary status.Read less <
Origin
Hal imported