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Disentangling the ISM phases of the dwarf galaxy NGC 4214 using [C II] SOFIA/GREAT observations

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The [CII] 158 um fine structure line is one of the dominant cooling lines in the interstellar medium (ISM) and is an important tracer of star formation. Recent velocity-resolved studies with Herschel/HIFI and SOFIA/GREAT showed that the [CII] line can constrain the properties of the ISM phases in st...

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Bibliographic Details
Main Authors: Fahrion, Katja (Author) , Cormier, Diane (Author) , Bigiel, Frank (Author) , Hony, Sacha (Author)
Format: Article (Journal) Chapter/Article
Language:English
Published: November 8, 2016
In: Arxiv

Online Access:Verlag, kostenfrei, Volltext: http://arxiv.org/abs/1611.02039
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Author Notes:K. Fahrion, D. Cormier, F. Bigiel, S. Hony, N.P. Abel, P. Cigan, T. Csengeri, U.U. Graf, V. Lebouteiller, S.C. Madden, R. Wu, and L. Young
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Disentangling the ISM phases of the dwarf galaxy NGC 4214 using [C II] SOFIA/GREAT observations by Fahrion, Katja (Author) , Cormier, Diane (Author) , Bigiel, Frank (Author) , Hony, Sacha (Author) ,


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