Initial highlights of the Herschel imaging survey of OB Young Stellar objects (HOBYS)
Résumé
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.