Astronomy and Astrophysics – Astrophysics
Scientific paper
Nov 2010
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010vaoa.conf...77n&link_type=abstract
"Evolution of Cosmic Objects through their Physical Activity, Proceedings of the Conference dedicated to Viktor Ambartsumian's 1
Astronomy and Astrophysics
Astrophysics
Scientific paper
Flare mechanism for explanation of relatively high energetic of flares in low mass red dwarf flare stars and fast course of flare processes is represented. The investigation was made on the base of existing observations of flare stars and ones obtained in the Abastumani Astrophysical Observatory. Spectral and photometrical observational peculiarities revealed during flares of the stars led us to the represented mechanism of flares. Discussion of mechanisms generating course of flare processes in the red dwarf flare stars is being continuing during half a century but improved understanding about a flare mechanism and excess energy source, which is generated during flare processes, is not reached yet. Our investigation is attempting to some degree supplement this gap.
Kochiashvili Nino
Natsvlishvili Rezo
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