Results 151 to 160 of about 215 (165)
Some of the next articles are maybe not open access.
2022
The problem of energetics of flare activity of dwarf stars in the lower main sequence of the Hertzsprung-Russell diagram is relevant in the context of the detection of powerful flares (superflares) and the possibility of assessing such phenomena on the Sun in the past and future. A brief historical review of the EV Lac original researches is presented,
Shlyapnikov, A.A., Gorbachev, M.A.
openaire +1 more source
The problem of energetics of flare activity of dwarf stars in the lower main sequence of the Hertzsprung-Russell diagram is relevant in the context of the detection of powerful flares (superflares) and the possibility of assessing such phenomena on the Sun in the past and future. A brief historical review of the EV Lac original researches is presented,
Shlyapnikov, A.A., Gorbachev, M.A.
openaire +1 more source
Astronomy Reports, 2001
We present spectral observations of the red-dwarf flare star EV Lac made at the Crimean Astrophysical Observatory in 1994 and 1995, and describe a method for semi-empirical modeling of the chromospheres of red dwarfs based on their emission spectra.
E. A. Baranovskii +2 more
openaire +1 more source
We present spectral observations of the red-dwarf flare star EV Lac made at the Crimean Astrophysical Observatory in 1994 and 1995, and describe a method for semi-empirical modeling of the chromospheres of red dwarfs based on their emission spectra.
E. A. Baranovskii +2 more
openaire +1 more source
Astrophysics, 1994
We studied the spectra of 24 flare stars of the Pleiades cluster region obtained on the 2.6m telescope of the Byurakan observatory in the years 1986–1989. From the spectral indices of titanium oxide (TiO) and other chemical elements of the stars investigated we determined their spectral classes and luminosities (absolute visual stellar magnitudes). The
L. V. Mirzoyan +2 more
openaire +1 more source
We studied the spectra of 24 flare stars of the Pleiades cluster region obtained on the 2.6m telescope of the Byurakan observatory in the years 1986–1989. From the spectral indices of titanium oxide (TiO) and other chemical elements of the stars investigated we determined their spectral classes and luminosities (absolute visual stellar magnitudes). The
L. V. Mirzoyan +2 more
openaire +1 more source
Coordinated observations of the red dwarf flare star EV Lac in 1998
2019The results of photometric studies of the flare star EV Lac obtained in the course of cooperative observations in 1998 are presented. No significant brightness variations in IR were found from simultaneous observations of the star in UBVRI and H bands, in coincidence with the observed optical flares.
Alekseev, I.Yu. +19 more
openaire +1 more source
Spectroscopic observations of red dwarfs I. Flare stars in the Pleiades
Astrophysics, 1991L. V. Mirzoyan +2 more
openaire +1 more source
Detection of a giant white-light flare on an L2.5 dwarf with the Next Generation Transit Survey
Monthly Notices of the Royal Astronomical Society: Letters, 2019Daniel Bayliss +2 more
exaly
The habitability of planets orbiting M-dwarf stars
Physics Reports, 2016Aomawa L Shields, John Asher Johnson
exaly
Flares of red dwarf stars and the galactic X-ray background
Astrophysics and Space Science, 1976N I Shakhovskaya
exaly

