Effect of the stellar inclination angle upon theoretical errors of l=1 p-mode parameters

Details Effect of the stellar inclination angle upon theoretical errors of l=1 p-mode parameters Effect of the stellar inclination angle upon theoretical errors of l=1 p-mode parameters

Jun 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008an....329..558b&link_type=abstract

Astronomische Nachrichten, Vol.329, Issue 5, p.558

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1

Methods: Data Analysis, Stars: Oscillations, Stars: Statistical

Scientific paper

The asteroseismic observations provided by current and future missions like CoRoT or Kepler will have a quality closer to those obtained for the Sun. In this context, tools and methods developed for helioseismology can be applied to other stars. In this paper, we focus on solar-like oscillations of stars with an unknown rotation axis inclination and study, by means of maximum-likelihood estimation, the errors on the determination of l=1 p-mode parameters.

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