S Dor variables (van Genderen+, 2001)

Details S Dor variables (van Genderen+, 2001) S Dor variables (van Genderen+, 2001)

Oct 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000ycat..33660508v&link_type=abstract

VizieR On-line Data Catalog: J/A+A/366/508. Originally published in: 2001A&A...366..508V

Physics

Stars: Supergiant, Stars: Variable, Photometry: Vbluw, Effective Temperatures, Magnitudes: Absolute, Reddening

Scientific paper

The goal in writing this paper is five fold: (1) to summarize the scientific achievements in the 20th century on S Dor variables (or LBVs); (2) to present an inventory of these variables in the Galaxy and the Magellanic Clouds with a description of their physical state and instability properties; (3) to emphasize the photometric achievements of the various types of instabilities. Generally this seems to be a neglected item resulting in a number of misunderstandings continuously wandering through literature; (4) to investigate the structure of the S Dor-area on the HR-diagram; (5) to estimate the total numbers of S Dor variables in the three stellar systems. (9 data files).

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