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

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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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Bibliographic Details
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
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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Summary:	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
Item Description:	Gesehen am 07.08.2020
Physical Description:	Online Resource
ISSN:	1365-2966
DOI:	10.1093/mnras/sty2507