Atmospheric velocity fields in tepid main sequence stars

Astronomy and Astrophysics

Volumn 503, Issue 3, 2009, Pages 973-984

  Landstreet, J D ^a,b   Kupka, F ^c,f   Ford, H A ^b,d,e   Officer, T ^b   Sigut, T A A ^b   Silaj, J ^b   Strasser, S ^b   Townshend, A ^b  

^a Armagh Observatory   (United States)

^b UNIVERSITY OF WESTERN ONTARIO   (Canada)

^c MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

^d SWINBURNE UNIVERSITY OF TECHNOLOGY   (Australia)

^e CSIRO   (Australia)

^f UNIVERSITÉ PARIS DIDEROT   (France)

Author keywords

[No Author keywords available]

Indexed keywords

AM STARS; ATMOSPHERIC CONVECTION; CONVECTIVE MOTIONS; EFFECTIVE TEMPERATURE; HIGH RESOLUTION; LINE PROFILES; LOCAL VELOCITY; MAIN SEQUENCE STARS; MICROTURBULENCE; MODEL SPECTRA; NUMERICAL SIMULATION; PARAMETER VALUES; SPECTRAL LINE; SPECTRAL LINE PROFILES; SPECTROSCOPIC SURVEYS; STELLAR ATMOSPHERES; STELLAR PARAMETERS; VELOCITY FIELD; WEAK LINES;

ABSORPTION; ATMOSPHERIC CHEMISTRY; COMPUTER SIMULATION; SPECTROSCOPY; VELOCITY;

STARS;

EID: 77954909560     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200912083     Document Type: Article

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