collaborators

5 papers

astro-ph.GA2010

From filamentary clouds to prestellar cores to the stellar IMF: Initial highlights from the Herschel Gould Belt survey

Ph. André, A. Men'shchikov, S. Bontemps +54

We summarize the first results from the Gould Belt survey, obtained toward the Aquila Rift and Polaris Flare regions during the 'science demonstration phase' of Herschel. Our 70-50…

astro-ph.GA2010

Physical properties of the Sh2-104 HII region as seen by Herschel

J. A. Rodón, A. Zavagno, J. -P. Baluteau +46

Context: Sh2-104 is a Galactic H ii region with a bubble morphology, detected at optical and radio wavelengths. It is considered the first observational confirmation of the collect…

astro-ph.SR2010

The Aquila prestellar core population revealed by Herschel

V. Könyves, Ph. André, A. Men'shchikov +37

The origin and possible universality of the stellar initial mass function (IMF) is a major issue in astrophysics. One of the main objectives of the Herschel Gould Belt Survey is to…

astro-ph.GA2010

The Herschel first look at protostars in the Aquila Rift

S. Bontemps, Ph. Andre, V. Konyves +40

As part of the science demonstration phase of the Herschel mission of the Gould Belt Key Program, the Aquila Rift molecular complex has been observed. The complete ~ 3.3deg x 3.3de…

astro-ph.GA2010

The physical properties of the dust in the RCW 120 HII region as seen by Herschel

L. D. Anderson, A. Zavagno, J. A. Rodon +41

Context. RCW 120 is a well-studied, nearby Galactic HII region with ongoing star formation in its surroundings. Previous work has shown that it displays a bubble morphology at mid-…