A superflare in EV Lacertae

Details A superflare in EV Lacertae A superflare in EV Lacertae

Apr 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982sval....8...85r&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 8, Mar. 1982, p. 163, 164.) Soviet Astronomy Letters, vol. 8, Mar.-Apr. 1982, p. 85, 86

Astronomy and Astrophysics

Astronomy

10

Flare Stars, Light Curve, Red Dwarf Stars, Stellar Flares, Electrophotometry, Magnitude, Ultraviolet Radiation

Scientific paper

The light curve of the great flare exhibited by EV Lac in July, 1980, which was of magnitude 6.4 and 4.5-hour duration, can be interpreted as a sum of two successive processes: a gradual, gentle flare and an enormous surge with a rapid flash. While subsequent observations have offered grounds for the belief that the flare observed was unique, it is noted that the observation has established that slow flares can occur in flaring field stars.

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