Accurate stellar rotational velocities using the Fourier transform of the cross correlation maximum

Astronomy and Astrophysics

Volumn 531, Issue , 2011, Pages

  Diaz C G ^a   Gonzalez J F ^a,b   Levato, H ^a,b   Grosso, M ^a,b  

^a UNIVERSIDAD NACIONAL DE SAN JUAN   (Argentina)

^b Facultad de Ciencias Naturales e Instituto M Lillo   (Argentina)

Author keywords

Methods: data analysis; Stars: fundamental parameters; Stars: rotation

Indexed keywords

BASE LINE; COMPUTATIONAL REQUIREMENTS; CROSS CORRELATIONS; CROSS-CORRELATION FUNCTION; HIGH PRECISION; HIGH-RESOLUTION SPECTRA; LIMB DARKENING; METHODS:DATA ANALYSIS; ROTATING STARS; ROTATIONAL VELOCITY; STARS: FUNDAMENTAL PARAMETERS; STARS: ROTATION; TYPICAL VALUES; WAVELENGTH DEPENDENCE;

DATA REDUCTION; MEASUREMENT ERRORS; METADATA; ROTATION; STARS;

FOURIER TRANSFORMS;

EID: 79959938964     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201016386     Document Type: Article

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