A statistical model of the light variability of the Insb-type star BN ORI

Details A statistical model of the light variability of the Insb-type star BN ORI A statistical model of the light variability of the Insb-type star BN ORI

Feb 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992kfnt....8...36p&link_type=abstract

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 8, Jan.-Feb. 1992, p. 36-41. In Russian.

Physics

Brightness Temperature, Light Curve, Statistical Analysis, Stellar Models, Stellar Spectra, Variable Stars, Histograms, Stellar Flares

Scientific paper

It is shown that the light variability of BN Ori observed in the past may be a result of the statistical addition of elementary light fadings which are commonly observed for antiflare stars. The possible number of elementary fadings is estimated at 3600. The increase in the frequency of antiflares, which is manifested in increased photometric activity, results in a lower level of mean brightness and an increased variability amplitude.

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