HILL, T.; MOTTE, F.; BONTEMPS, Sylvain; ZAVAGNO, Annie; SCHNEIDER, N.; HENNEMANN, M.; DI FRANCESCO, J.

Metadatos

Licencia de uso del documento

HILL, T.
Astrophysique Interprétation Modélisation [AIM (UMR7158 / UMR_E_9005 / UM_112)]

MOTTE, F.
Astrophysique Interprétation Modélisation [AIM (UMR7158 / UMR_E_9005 / UM_112)]
Institut de Recherches sur les lois Fondamentales de l'Univers [IRFU]

BONTEMPS, Sylvain
FORMATION STELLAIRE 2010

Idioma

Communication dans un congrès

Este ítem está publicado en

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

Resumen en inglés

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.< Leer menos

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Centros de investigación

Laboratoire d'Astrophysique de Bordeaux (LAB) - UMR 5804