Flaring red dwarfs and stellar activity of the solar type - half a century of researches in the Crimean Astrophysical Observatory

  • R.E. Gershberg Crimean Astrophysical Observatory, Nauchny, 298409

Abstract

The basic results of long-term researches of flaring stars in the Crimean Astrophysical Observatory are given: photoelectric monitoring of the known and suspected flaring stars, nebular and chromospheric models of flares, spectral observations of flares with a high time resolution, co-operative photometric observations and time distribution of stellar flares, distribution of flares along energy and power spectra of flares, spectra of flaring stars in a quiet state, observations for EV Lac during the international co-operative programs and from the space station ASTRON, high-speed photometry and colorimetry of flares, polarimetry observations, research spottedness of stars and the zone model of stellar spottedness, long cycles of activity, magnetometric observations. There has been carried out and is being supported the cataloguing of M to G - F-type flaring stars. 

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Published
2017-12-14
How to Cite
Gershberg R., 2017. Izvestiya Krymskoi Astrofizicheskoi Observatorii, vol. 113, no. 1, pp. 36-77. Available at: https://jn.craocrimea.ru/index.php/izvcrao/article/view/447 (Accessed: 1December2020)
Section
Research articles

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