A correlation between the age of a stellar aggregate and the color parameters of its member flare stars

Details A correlation between the age of a stellar aggregate and the color parameters of its member flare stars A correlation between the age of a stellar aggregate and the color parameters of its member flare stars

Feb 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982sval....8...19g&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 8, Jan. 1982, p. 38-42.) Soviet Astronomy Letters, vol. 8, Jan.-Feb. 1982, p. 19-22. Tr

Astronomy and Astrophysics

Astronomy

4

Flare Stars, Stellar Color, Stellar Evolution, T Tauri Stars, Ubv Spectra, H Alpha Line, Herbig-Haro Objects, Main Sequence Stars

Scientific paper

An empirical relation is established between the mean departure from the
main sequence in the two-color (U-B, B-V) diagram (along the U-B axis)
of a system of flare stars of H-alpha emission stars and the age of the
aggregate containing that system (or of the nonstable stars belonging to
the aggregate). The ages of four T Tau stars are estimated.

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