On deriving p-mode parameters for inclined solar-like stars

Astronomy and Astrophysics

Volumn 486, Issue 3, 2008, Pages 867-875

  Ballot, J ^a   Appourchaux, T ^b   Toutain, T ^c   Guittet, M ^a  

^a MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

^b UNIVERSITÉ PARIS SUD   (France)

^c UNIVERSITY OF BIRMINGHAM   (United Kingdom)

Author keywords

Methods: data analysis; Methods: statistical; Stars: oscillations

Indexed keywords

CORRELATION METHODS; ERRORS; HOSE FITTINGS; MONTE CARLO METHODS; SOLAR ENERGY; SOLAR SYSTEM;

ANALYTICAL APPROXIMATIONS; CENTRAL FREQUENCY (CF); HELIOSEISMOLOGY; HESSIAN MATRICES; HIGH QUALITY (HQ); MAXIMUM LIKELIHOOD (MLET); MONTE CARLO SIMULATION (MCS); ROTATION AXES; ROTATIONAL SPLITTING; SEMI-ANALYTICAL; SOLAR LIKE OSCILLATIONS; SOLAR-LIKE STARS; TOTAL POWER;

ERROR ANALYSIS;

EID: 47749129559     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20079343     Document Type: Article

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