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Herschel Galactic Cold Cloud Core Analysis

Published online by Cambridge University Press:  21 March 2013

Erika Verebelyi  and
Laurent Pagani
Erika Verebelyi
Affiliation:
Eötvös Loránd University, Pázmány Péter sétány 1/A, H-1117 Budapest, Hungary email: everebelyi@astro.elte.hu
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Abstract

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We have compiled a sample of 106 lesser-known cores from the Herschel Galactic Cold Cloud Cores Key Program (Juvela, M. et al. 2007). Based on the assumption, that these represent the crowd of the cold cores in the galaxy well, we have started a deep individual investigation, beginning with a ground-based follow-up and molecular line measurement at IRAM 30m telescope. We present the methods and calculated values of the most important parameters on a selected source: the G130.38+11.25 molecular cloud, which is part of the L1340.

Keywords

ISM: clouds — dustextinction — ISM: molecules
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 8 , Symposium S292: Molecular Gas, Dust, and Star Formation in Galaxies , August 2012 , pp. 115
Copyright
Copyright © International Astronomical Union 2013

References

Juvela, M.et al. 2012, A&A, 541A, 12JGoogle Scholar
Roman-Duval, J.et al. 2010, ApJ 723 492–507CrossRefGoogle Scholar
Van der Tak, F. F. S.et al. 2007, A&A, 468, 627Google Scholar