2008/04/28 by W. J. Chaplin, G. Houdek, T. Appourchaux +3 · 76 citations
Physics and Astronomy · #Asteroseismology #Astronomy and Astrophysical Research #Cepheid variable #Kepler #Scientific Research and Discoveries #Stars #Stellar, planetary, and galactic studies #Variable star #astro-ph
paper · pdf · doi:10.1051/0004-6361:200809695
published in Astronomy and Astrophysics 485(3), 813-822 (EDP Sciences) · 11 pages; accepted for publication in A&A. Corrections to a few minor typos. Changes to plots to make bold symbols clearer in on-screen PDF
openalex publication_date 2008/04/28 · arxiv created 2008/05/22 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05
Context. Asteroseismology of Sun-like stars is undergoing rapid expansion with, for example, new data from the CoRoT mission and continuation of ground-based campaigns. There is also the exciting upcoming prospect of NASA's Kepler mission, which will allow the asteroseismic study of several hundred Sun-like targets, in some cases for periods lasting up to a few years.