Flares of Orion-Population variables in the Taurus T3 association

Details Flares of Orion-Population variables in the Taurus T3 association Flares of Orion-Population variables in the Taurus T3 association

Oct 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987afz....27..207k&link_type=abstract

Astrofizika (ISSN 0571-7132), vol. 27, Oct. 1987, p. 207-217. In Russian.

Astronomy and Astrophysics

Astronomy

1

Astronomical Photography, Flare Stars, Stellar Flares, T Tauri Stars, Variable Stars, Light Curve, Molecular Clouds, Orion Constellation, Ultraviolet Astronomy

Scientific paper

Thirteen new flare stars, proved to be irregular variables of the Orion Population, were discovered. Seventeen flares on these stars were detected for about 750 hours of the effective observing time. A great variety and multiplicity and various dynamics of flare energy release processes are shown. The existence of flare stars with some properties typical for both of the T Tauri and UV Ceti stars simultaneously indicates an intimate relation between the above mentioned types of young nonstable stars. The population of flare stars in the Taurus Dark Cloud region is apparently as young as in Orion and Monoceros.

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