2008/10/01 by N. J. Tarrant, W. J. Chaplin, Y. P. Elsworth +2 · 9 citations
Engineering · Physics and Astronomy · Social Sciences · #Apparent magnitude #Binary star #Educational Leadership and Practices #Observable #Solar mass #Space Technology and Applications #Star (game theory) #Stars #Stellar evolution #Stellar mass #Stellar, planetary, and galactic studies #astro-ph
paper · pdf · doi:10.1051/0004-6361:200810952
published in Astronomy and Astrophysics 492(1), 167-169 (EDP Sciences) · 3 pages, 4 figures. Accepted for publication in A&A
openalex publication_date 2008/10/01 · arxiv created 2008/10/21 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05
Aims. As g-mode pulsators, gamma-Doradus-class stars may naïvely be expected to show a large number of modes. Taking advantage of the long photometric time-series generated by the solar mass ejection imager (SMEI) instrument, we have studied the star gamma Doradus to determine whether any other modes than the three already known are present at observable amplitude.