3D spectral synthesis and rotational line broadening (Research Note)

Astronomy and Astrophysics

Volumn 471, Issue 3, 2007, Pages 925-927

  Ludwig, H G ^a  

^a UNIVERSITÉ PARIS DIDEROT   (France)

Author keywords

Hydrodynamics; Line: profiles; Methods: numerical; Radiative transfer; Stars: atmospheres

Indexed keywords

OPTICAL RESOLVING POWER; RADIATIVE TRANSFER; ROTATION; STARS;

LINE: PROFILES; METHODS: NUMERICAL; STARS: ATMOSPHERES;

SPECTRUM ANALYSIS;

EID: 34548097892     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20066909     Document Type: Article

References (5)

1. Caffau, E., Ludwig, H.-G., Steffen, M., et al. 2007, A&A, in preparation
2. Dravins, D., & Nordlund, Å. 1990, A&A, 228, 203
3. Gray, D. F. 1992, in The observation and analysis of stellar photospheres, 2nd ed. (Cambridge University Press)
4. Huang, S.-S. 1961, ApJ 133, 130
5. Reiners, A., & Schmitt, J. H. M. M. 2002, A&A, 384, 155