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: | , , , |
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| Format: | Article (Journal) |
| Language: | English |
| Published: |
2018 September 18
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| 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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| 520 | |a 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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