On the feasibility of chemical modeling of a proplanetary disk

Baltic Astronomy

Volumn 13, Issue 3, 2004, Pages 454-458

  Semenov, D ^a,b   Pavlyuchenkov, Ya ^c   Henning, Th ^b   Herbst, E ^d   Van Dishoeck, E ^e  

^a Astrophysical Institute and University Observatory (AIU)   (Germany)

^b MAX PLANCK INSTITUT FÜR ASTRONOMIE   (Germany)

^c INSTITUTE OF ASTRONOMY   (Russian Federation)

^d OHIO STATE UNIVERSITY   (United States)

^e LEIDEN UNIVERSITY   (Netherlands)

Author keywords

Astrochemistry; Line: profiles; Planetary systems: protoplanetary disks; Radiative transfer

Indexed keywords

EID: 18444398633     PISSN: 13920049     EISSN: None     Source Type: Journal    
DOI: None     Document Type: Article

References (9)

1. Aikawa Y., Herbst E. 1999, A&A, 351, 233
2. Aikawa Y., van Zadelhoff G.-J., van Dishoeck E. F., Herbst E. 2002, A&A, 386, 622
3. D'Alessio P., Calvet N., Hartmann L. et al. 1999, ApJ, 527, 893
4. Draine B. T. 1978, ApJS, 36, 595
5. Li Z.-Y., Shematovich V. I., Wiebe D. S., Shustov B. M. 2002, ApJ, 569, 792
6. Millar T. J., Farquhar P. R. A., Willacy K. 1997, A&AS, 121, 139
7. Pavlyuchenkov Ya., Shustov B. M. 2004, Astronomy Reports, in press
8. Semenov D. A., Wiebe D. S., Henning Th. 2004, A&A, 417, 93
9. Wiebe D. S., Semenov D. A., Henning Th. 2003, A&A, 399, 197