Work

The relative number of flare stars in systems of different ages

Year: 1990

Type: conference-paper

Abstract: The problem of flare activity frequency among red dwarf stars is discussed. The observational data on stars in Orion, Pleiades and solar vicinity are used. It is shown, that relative number of flare stars among all red dwarf stars in the considered samples is increasing towards the lower luminosity stars. The flare stars are found in the considered samples begining with a definite luminosity, this limiting luminosity being decreased with the aging of the system which includes flare stars. A possible explanation of the observed phenomenon is given.

Source: Symposium - International Astronomical Union

DOI: 10.1017/s0074180900187583

Authors: V.V. Hambarian, A.T. Garibjanian, L.V. Mirzoyan, A.L. Mirzoyan

Institution: Byurakan Astrophysical Observatory

Language: English

Topic: Stellar, planetary, and galactic studies

Subfield: Astronomy and Astrophysics

Field: Physics and Astronomy

Domain: Physical Sciences

Open Access status: bronze

OpenAlex ID: W158790282

FWCI:

Cites: 8

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Related to: 10