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Catalog Service:
Beta Cephei stars in the ASAS-3 data. I.

Short name: J/A+A/477/907
IVOA Identifier: ivo://CDS.VizieR/J/A+A/477/907
DOI (Digital Object Identifier): 10.26093/cds/vizier.34770907
Publisher: CDS[+][Pub. ID]
More Info: https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/477/907
VO Compliance: Level 2: This is a VO-compliant resource.
Status: active
Registered: 2008 Mar 26 22:26:25Z
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Description


We analyse V-filter photometry of 41 known Beta 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. We detected amplitude changes in three Beta Cephei stars, BW Cru, V836 Cen, and V348 Nor. Period changes were found in KK Vel and V836 Cen. Our analysis shows that intrinsic period changes are more common among multiperiodic stars, apparently because they are caused by some kind of mode interaction. In addition, we found new modes for seven stars, and for ten others we provide new solutions or remove ambiguities in the detected frequencies. One candidate hybrid Beta Cephei/SPB star, HD 133823, is discovered.

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