Flare stars in star clusters and the faint end of the stellar luminosity function.

Details Flare stars in star clusters and the faint end of the stellar luminosity function. Flare stars in star clusters and the faint end of the stellar luminosity function.

Jul 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995pobeo..49...57s&link_type=abstract

Publications de l'Observatoire Astronomique de Beograd, No. 49, p. 57 - 62

Astronomy and Astrophysics

Astronomy

Flare Stars: Star Clusters, Flare Stars: Luminosity Function, Flare Stars: Photometric Properties

Scientific paper

Flare stars belong to the red dwarfs, the faintest stellar objects known, dK and dM stars contribute about half of the total stellar mass in the solar vicinity. They are a kind of dark matter candidates. Probably at least half of these stars are flare stars which can be detected (during high amplitude outbursts) at a significantly larger distance. This fact makes these faint objects and their investigation exceptionally important. The results of a two decades long photometric and astrometric programme are summarized below.

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