β Cephei stars in the ASAS-3 data

2007/11/20 by A. Pigulski, G. Pojmański, G. Pojmanski · 19 citations
Engineering · Physics and Astronomy · #Amplitude #Astro and Planetary Science #Astronomical Observations and Instrumentation #Astronomy #Astrophysics #Context (archaeology) #Optics #Photometry (optics) #Physics #Stars #Stellar, planetary, and galactic studies #astro-ph

paper · pdf · doi:10.1051/0004-6361:20078580

published in Astronomy and Astrophysics 477(3), 907-915 (EDP Sciences) · 22 pages, 11 figures, accepted for publication in A&A

arxiv created 2007/11/20 · openalex publication_date 2007/12/04 · arxiv updated 2009/12/01 · openalex created_date 2022/09/23 · openalex updated_date 2026/07/31

Abstract

Aims.We analyse V-filter ASAS-3 photometry of 41 known β Cephei-type stars. The ASAS-3 photometry is combined with the archival data, if available, to determine long-term stability of periods and amplitudes of excited modes.

Citations

• Asteroseismological studies of three Cephei stars: IL Vel, V433 Car and KZ Mus