The far infrared line spectrum of the protostar IRAS 16293-2422

Astronomy and Astrophysics

Volumn 331, Issue 1, 1998, Pages 372-382

  Ceccarelli, C ^a,b   Caux, E ^c   White, G J ^d   Molinari, S ^b,e   Furniss, I ^f   Liseau, R ^g   Nisini, B ^b   Saraceno, P ^b   Spinoglio, L ^b   Wolfire, M ^h,i  

^a LABORATOIRE D ASTROPHYSIQUE   (France)

^b CNR   (Italy)

^c IRAP   (France)

^d QUEEN MARY UNIVERSITY OF LONDON   (United Kingdom)

^e ISO Science Operations Centre   (Spain)

^f UNIVERSITY COLLEGE LONDON   (United Kingdom)

^g STOCKHOLM OBSERVATORY   (Sweden)

^h UNIVERSITY OF MARYLAND   (United States)

ⁱ TOWSON UNIVERSITY   (United States)

Author keywords

Infrared: ISM: lines; ISM: individual: IRAS 16293 2422; ISM: jets and outflows; Stars: formation

Indexed keywords

EID: 0000013772     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: None     Document Type: Article

References (50)

1. André P., Ward-Thompson D., Barsony, M., 1993, ApJ 406, 122
2. Blake, G.A, van Dishoeck E., Jansen D.J., Groesbeck T.D., Mundy, L.G. 1994, ApJ 428, 680
3. Ceccarelli C., Hollenbach D.J., Tielens A.G.G.M., 1996, ApJ 471, 400
4. Ceccarelli C., Haas M.R., Hollenbach D.J., Rudolph A.L., 1997, ApJ 476, 771
5. Cohen M., Hollenbach D.J., Haas M.R., Erickson E.F., 1988, ApJ 329, 863
6. van Dishoeck E.F., Blake G.A., Jansen D.J., Groesbeck T.D., 1995, ApJ 447, 760
7. Doty S.D., Neufeld D.A., 1997, ApJ, in press
8. Draine, B.T., 1980, ApJ 241, 1021
9. Fukui Y., Sugitani K., Takaba H., et al. 1986, ApJ 311,L85
10. Glassgold A.E., Mannon G.A., Huggins P.J., 1991, ApJ 373, 254
11. Graff M.M., Dalgamo A., 1987, ApJ 317, 432
12. Green S., Malauendes S., McLean A.D., 1993, ApJS 85, 181
13. Gregersen E.M., Evans N.J.II, Zhou S., Choi M., 1997, ApJ 484, 256
14. Hollenbach D.J. ,Tielens A.G.G.M. Takahashi, T., 1991 (HTT91), ApJ 377., 192
15. Hollenbach D.J., McKee C.F., 1989, ApJ 342, 306
16. Kaufman M.J., Neufeld D.A., 1996, ApJ 456, 611
17. Keene J., 1990, in: Proceedings of SETI conference "Carbon in the Galaxy: Studies from Earth and Space", p 181-196 (SEE N90-27562 21-88)
18. Langer W.D., Graedel T.E., Frerking M.A., Armentrout, P.B., 1984, ApJ 277, 581
19. Lefloch B., Lazareff B., 1995, A&A 301, 522
20. Li Z.Y., Shu F.H., 1996, ApJ 468, 261
21. Liseau R., Ceccarelli C., Larsson B., 1996, A&A. 315, L181
22. Lizano S., Giovannardi C., 1995, ApJ 447, 742
23. McKee C.F., Storey J.W.V., Watson D.M., Green S., 1982, ApJ 259, 647
24. Mizuno A., Fukui Y., Iwata T., Nozawa S., Takano T., 1990, ApJ 356, 184
25. Mundy L.G., Wootten A., Wilking B.A., Blake G.A. Sargent A.I., 1992, ApJ 385, 306
26. Nelson R.P., Langer W.D., 1997, ApJ 482, 796
27. Nisini B., Lorenzetti D., Cohen M. et al, 1996, A&A, 315, L32
28. Offer A.R., van Hemert M.C., van Dishoeck E.F., 1994, J.Chem.Phys. 100, 362
29. Raga A., Cabrit S., 1993, A&A 278, 267
30. Rothman L.S. et al, 1987, Appl. Opt. 26, 4058
31. Saraceno P., Ceccarelli C., Clegg P.E. et al, 1996a, A&A, 315, L293
32. Saraceno P., Andre' P., Ceccarelli C., Griffin M., Molinari S., 1996b, A&A 309, 827
33. Shematovich V., Shustov B., Wiebe D., 1997, A&A preprint
34. Shu F.H., 1977, ApJ 214, 488
35. Shu F.H., Najita J., Ruden S., Lizano S., 1994, ApJ 429, 797
36. Stahler S.W., 1988, ApJ 332, 804
37. Stahler S.W., 1994, ApJ 422, 616
38. Swinyard B.M., Clegg P.E., Ade P.A.R. et al., 1996, A&A 315, L43
39. Tielens A.G.G.M., Hollenbach D.J., 1985, ApJ 291, 747
40. van Dishoeck E.F., Blake G.A., Jansen D.J., Groesbeck T.D., 1995, ApJ 447, 760
41. Walker C., Lada C.J., Young E.T., Margulis M., Wilking B.A., 1985, BAAS 17, 835
42. Walker C., Lada C.J., Young E.T., Margulis M., 1988, ApJ 332, 335
43. Walker C.K., Carlstrom J.E., Bieging J.H., Lada C.J., Young E.T., 1990, ApJ 364, 173
44. Walker C., Carlstrom J.E., Bieging J.H., 1993, ApJ 402, 655
45. Wolfire M.G., Tielens A.G.G.M., Hollenbach D.J., 1990, ApJ 358, 116
46. Wootten A., 1989, ApJ 337, 858
47. Wootten A., Loren R.B., 1987, ApJ 317, 220
48. Yui Y.Y., Nakagawa T., Doi Y., et al., 1993, ApJ 419, L37
49. Zhou S., 1992, ApJ 394, 204
50. Zhou S., 1995, ApJ 442, 685