Spherically symmetric model atmospheres for low-mass pre-main-sequence stars with effective temperatures between 2000 and 6800 K

Astrophysical Journal

Volumn 539, Issue 1 PART 1, 2000, Pages 366-371

  Allard, France ^a   Hauschildt, Peter H ^b   Schweitzer, Andreas ^b  

^a UNIVERSITÉ DE LYON   (France)

^b UNIVERSITY OF GEORGIA   (United States)

Author keywords

Stars: atmospheres; Stars: late type; Stars: low mass, brown dwarfs; Stars: pre main sequence

Indexed keywords

EID: 0034632325     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/309218     Document Type: Article

References (10)

1. Allard, F., Hauschildt, P. H., & Schwenke, D. 2000, ApJ, in press
2. Baraffe, I. et al. 2000, in preparation
3. Hauschildt, P., Allard, F., Ferguson, J., Baron, E., & Alexander, D. R. 1999, ApJ, 525, 871 (NG giant)
4. Hauschildt, P. H., Allard, F., & Baron, E. 1999, ApJ, 512, 377
5. Hauschildt, P. H., & Baron, E. 1999, J. Comput. Appl. Math., 102, 41
6. Jaschek, C., & Jaschek, M. 1995, The Behavior of Chemical Elements in Stars (Cambridge: Cambridge Univ. Press)
7. Leggett, S. K., Allard, F., Dahn, C., Hauschildt, P. H., Kerr, T. H., & Rayner, J. 1999, ApJ, 535, 965
8. Leinert, C., Allard, F., Richichi, A., & Hauschildt, P. H. 1999, A&A, 353, 691
9. Partridge, H., & Schwenke, D. W. 1997, J. Chem. Phys., 106, 4618
10. Schwenke, D. W. 1998, Faraday Discuss., 109, 321