Some Statistical Properties of Short Flares of Flare Stars

Details Some Statistical Properties of Short Flares of Flare Stars Some Statistical Properties of Short Flares of Flare Stars

Oct 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997rmxaa..33..107t&link_type=abstract

Revista Mexicana de Astronomia y Astrofisica, 33, p. 107- 115 (1997)

Astronomy and Astrophysics

Astronomy

3

Scientific paper

Several flares were detected in the flare stars EV Lac and V 577 Mon in high time resolution observations carried out with the 40-cm telescope at Byurakan, the 1-m telescope of the OAN in Tonantzintla, and the 2.1-m telescope of the INAOE in Cananea. About half of the detected flares are of the spiky type with a total duration less than 1 sec. It is shown that the spiky flares which occur mostly after normal, longer lasting flares are systematically bluer than the preceding main flares.

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