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- W2017130835 abstract "Thirteen new flare stars that are irregular variables of the Orion population have been found in an investigation of the Taurus Dark Cloud region by the homogeneous photographic multiexposure method using wide-angle Schmidt telescopes of the Byurakan Astrophysical Observatory. About 750 h of effective observation time led to the discovery of 17 flares in these stars. Analysis of the complicated light curves of the flares of these stars indicates a variety and multiplicity of phenomena and different dynamics of the energy release processes during the flares. The existence of flare stars that simultaneously exhibit the properties of T Tau and UV Cet type indicates that there is an intimate relationship between these types of young nonstationary stars. The flare star population in the region of the Taurus Dark Cloud is in all probability as young as the analogous groups of stars in Orion and Monoceros." @default.
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- W2017130835 date "1988-01-01" @default.
- W2017130835 modified "2023-09-27" @default.
- W2017130835 title "Flares of Orion population variables in the association Taurus T3" @default.
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- W2017130835 doi "https://doi.org/10.1007/bf01006004" @default.
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