Flare activity variations on stars of different ages comparable to those of the sun

Details Flare activity variations on stars of different ages comparable to those of the sun Flare activity variations on stars of different ages comparable to those of the sun

Aug 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990ap%26ss.170...63s&link_type=abstract

(IAU, European Regional Astronomy Meeting, 11th, La Laguna, Spain, July 3-8, 1989) Astrophysics and Space Science (ISSN 0004-640

Astronomy and Astrophysics

Astrophysics

3

Astronomical Photometry, K Stars, M Stars, Stellar Flares, Dwarf Stars, Flare Stars, Spectral Resolution, Stellar Evolution, Time Dependence

Scientific paper

More than 1500 flare-ups of stars of the Eta Tauri fields were statistically investigated and flare activity variations of the most active objects were analyzed. Such variations seem to be usual rather than exceptional. Although observational selection effects raised difficulties, a new method developed in order to exempt from dubious data was tested successfully and used regularly. It was found that activity variations of dwarfs stars are common on younger and older objects too. Time-dependence of these phenomena is reminiscent of the solar white-light flare occurrence.

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