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Results from the Herschel Gould Belt Survey in the Ophiuchus Main Cloud

Part of: IAU Issue 315 - From Interstellar Clouds...

Published online by Cambridge University Press:  12 September 2016

Bilal Ladjelate ,
Philippe André ,
Vera Könyves ,
Alexander Men'shchikov  and
the HGBS team
Bilal Ladjelate
Affiliation:
Service d'Astrophysique, AIM, CEA Saclay, 91191, Gif-sur-Yvette, France email: [email protected]
Philippe André
Affiliation:
Service d'Astrophysique, AIM, CEA Saclay, 91191, Gif-sur-Yvette, France email: [email protected]
Vera Könyves
Affiliation:
Service d'Astrophysique, AIM, CEA Saclay, 91191, Gif-sur-Yvette, France email: [email protected]
Alexander Men'shchikov
Affiliation:
Service d'Astrophysique, AIM, CEA Saclay, 91191, Gif-sur-Yvette, France email: [email protected]
the HGBS team
Affiliation:
http://gouldbelt-herschel.cea.fr
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Abstract

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As part of the Herschel Gould Belt Survey (HGBS), the Ophiuchus molecular cloud was imaged in the submillimeter range. Here, we summarize and briefly discuss the main results.

Keywords

stars: formationmass functionISM: structure
Type
Poster Papers
Information
Proceedings of the International Astronomical Union , Volume 11 , Symposium S315: From Interstellar Clouds to Star-Forming Galaxies: Universal Processes? , August 2015 , E46
Copyright
Copyright © International Astronomical Union 2016 

References

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