Non-LTE line formation in clumpy and turbulent molecular clouds

Astronomy and Astrophysics

Volumn 359, Issue 1, 2000, Pages 405-412

  Hegmann, M ^a   Kegel, W H ^a  

^a GOETHE UNIVERSITY   (Germany)

Author keywords

ISM: clouds; ISM: Molecules; Line: formation; Radiative transfer; Radio lines: ISM

Indexed keywords

EID: 0000456380     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: None     Document Type: Article

References (16)

1. Albrecht M.A., Kegel W.H., 1987, A&A 176, 317
2. Black J.H., Willner S.P., 1984, ApJ 279, 673
3. Flower D.R., Launay J.M., 1985, MNRAS 214, 271
4. Gail H.P., Hundt E., Kegel W.H., et al., 1974, A&A 32, 65
5. Gail H.P., Sedlmayr E., 1974a, A&A 36, 17
6. Gail H.P., Sedlmayr E., Traving G., 1975, A&A 44, 421
7. Gail H.P., Sedlmayr E., Traving G., 1980, J. Quant. Spectr. Radiat. Transfer 23, 267
8. Hegmann M., Kegel W.H., 1996, MNRAS 283, 167
9. Juvela M., 1996, A&A 322, 943
10. Kegel W.H., Piehler G., Albrecht M.A., 1993, A&A 270, 407
11. Pagani L., 1997, A&A 333, 269
12. Park Y.-S., Hong S.S., 1995, A&A 300, 890
13. Piehler G., Kegel W.H., 1994, A&A 297, 841
14. Risken H., 1988, The Fokker-Planck Equation. Berlin Heidelberg: Springer
15. Spitzer L., 1978, Physical Processes in the Interstellar Medium. New York: Wiley-Interscience
16. Traving G., 1980, A&A 85, 281