Physics
Scientific paper
Jan 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985nascp2358...62b&link_type=abstract
In NASA. Goddard Space Flight Center The Origin of Nonradiative Heating/Momentum in Hot Stars p 62-65 (SEE N85-17755 08-88)
Physics
1
B Stars, Stellar Flares, Stellar Luminosity, Galactic Clusters, Photometry, Stellar Envelopes, Variations
Scientific paper
Light variations of the B-type star HD 160202 in the galactic cluster M6 are presented. A flare type increase in brightness by about three magnitudes in a time interval of 40 minutes was recorded. It is shown that a B-type star in the galactic cluster M 6 went through the process of shell formation and a flare type increase in brightness in a time interval of three years. Similar cases associated with B-type stars were reported in the past; however, they represent sporadic and accidental observations. The observations presented here show a flare-type event with a resolution of five minutes.
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