The limb-darkening for spherically symmetric NextGen model atmospheres: A-G main-sequence and sub-giant stars

Astronomy and Astrophysics

Volumn 412, Issue 1, 2003, Pages 241-248

  Claret, A ^a   Hauschildt, P H ^b  

^a INSTITUTO DE ASTROFÍSICA DE ANDALUCÍA CSIC   (Spain)

^b UNIVERSITY OF HAMBURG   (Germany)

Author keywords

Stars: atmospheres; Stars: binaries: eclipsing

Indexed keywords

GRAVITATION; INTERFEROMETRY; LEAST SQUARES APPROXIMATIONS; MATHEMATICAL MODELS; PARAMETER ESTIMATION; PLANETS; TURBULENCE;

FLUX CONSERVATION; STARS;

ASTROPHYSICS;

EID: 0346332700     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20031405     Document Type: Article

References (8)

1. Claret, A. 1998, A&A, 335, 653
2. Claret, A. 2000, A&A, 363, 1081
3. Claret, A. 2003, A&A, 401, 657
4. Hauschildt, P. H., Allard, F., & Baron, E. 1999, ApJ, 512, 377
5. Hauschildt, P. H., Allard, F., Ferguson, J., Baron, E., & Alexander, D. R. 1999, ApJ, 525, 871
6. Hauschildt, P. H., & Baron, E. 1999, J. Comput. Appl. Math., 102, 41
7. Kurucz, R. 1993, Series of CDROMs
8. Orosz, J. A., & Hauschildt, P. H. 2000, A&A, 364, 265