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Monthly Notices of the Royal Astronomical Society

Volumn 369, Issue 3, 2006, Pages 1281-1286

Rotation speed and stellar axis inclination from p modes: How CoRoT would see other suns

(3) Ballot, J a,c Garcia R A a,b Lambert, P a,b

a UNIVERSITÉ PARIS DIDEROT (France)

b CEA SACLAY (France)

c MAX PLANCK INSTITUT FÜR ASTROPHYSIK (Germany)

Author keywords

Methods: data analysis; Stars: oscillations; Stars: rotation; Sun: helioseismology

Indexed keywords

INTELLIGENT SYSTEMS; MONTE CARLO METHODS; ROTATION RATE;

AXIS INCLINATION; METHODS. DATA ANALYSIS; ROTATION AXES; ROTATION RATE; ROTATION SPEED; SOLAR ROTATION; STAR OSCILLATIONS; STARS: ROTATION; STELLARS; SUN: HELIOSEISMOLOGY;

STARS;

EID: 33745142201 PISSN: 00358711 EISSN: 13652966 Source Type: Journal
DOI: 10.1111/j.1365-2966.2006.10375.x Document Type: Article

Times cited : (93)

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