2006/10/06 by V. Ripepi, S. Bernabei, M. Marconi +7 · 1 citation
Physics and Astronomy · #Astronomy and Astrophysical Research #Herbig Ae/Be star #Herbig–Haro object #O-type star #Scientific Research and Discoveries #Star (game theory) #Stars #Stellar evolution #Stellar mass #Stellar, planetary, and galactic studies #T Tauri star #Variable star #astro-ph
paper · pdf · doi:10.1051/0004-6361:20065728
A&A Accepted, 10 pages + 4 pages online material
arxiv created 2006/10/06 · openalex publication_date 2006/11/13 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05
Context.The study of pulsation in pre-main-sequence intermediate mass stars represents an important tool for deriving information on the stellar parameters and structure, as well as for testing the validity of current theoretical models. The interest in this class of variable stars has significantly increased during the last decade and about 30 members are presently known in the literature.