Gamma-bursts and flares on red dwarfs.

Details Gamma-bursts and flares on red dwarfs. Gamma-bursts and flares on red dwarfs.

May 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989atsir1537...17a&link_type=abstract

Astronomicheskii Tsirkulyar, No. 1537, p. 17 - 18

Astronomy and Astrophysics

Astronomy

Red Dwarfs: Stellar Flares, Flare Stars: Gamma-Ray Bursts, Stellar Flares: Gamma-Ray Bursts, Red Dwarfs: Gamma-Ray Bursts

Scientific paper

High-temperature dense plasma is the source of γ-radiation. This plasma can be formed in upper layers of a star due to processes of magnetic compression of closed magnetic configurations with low plasma β and under a local magnetic field of order 30 kGs. On the stage of stretching development plasma temperature and density increase and can achieve thermonuclear values. This impulsive radiation of stretching of pinch-column can ensure agreement with observational data. It is remarkable that in this model the optical flare must precede the X- and γ-rays' flares.

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