Synthetic [CII] emission maps of a simulated molecular cloud in formation

Abstract. The C+ ion is an important coolant of interstellar gas, and so the [C ii] fine structure line is frequently observed in the interstellar medium. Howe

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Main Authors: Franeck, Annika (Author) , Glover, Simon (Author) , Klessen, Ralf S. (Author) , Pellegrini, Eric William (Author)
Format: Article (Journal)
Language:English
Published: 2018 September 18
In: Monthly notices of the Royal Astronomical Society
Year: 2018, Volume: 481, Issue: 4, Pages: 4277-4299
ISSN:1365-2966
DOI:10.1093/mnras/sty2507
Online Access:Verlag, Volltext: http://dx.doi.org/10.1093/mnras/sty2507
Verlag, Volltext: https://academic.oup.com/mnras/article/481/4/4277/5101459
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Author Notes:A. Franeck, S. Walch, D. Seifried, S.D. Clarke, V. Ossenkopf-Okada, S.C.O. Glover, R. S. Klessen, P. Girichidis, T. Naab, R. Wünsch, P.C. Clark, E. Pellegrini and T. Peters

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