Interpretation of photometric observations of R Coronae Borealis - The light curves

Details Interpretation of photometric observations of R Coronae Borealis - The light curves Interpretation of photometric observations of R Coronae Borealis - The light curves

Dec 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990azh....67.1280p&link_type=abstract

Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 67, Nov.-Dec. 1990, p. 1280-1287. In Russian.

Astronomy and Astrophysics

Astronomy

5

Light Curve, R Coronae Borealis Stars, Stellar Spectrophotometry, Astronomical Models, Cosmic Dust, Interstellar Extinction, Interstellar Matter, Stellar Radiation

Scientific paper

Calculations confirm the eruptive hypothesis according to which the light variability of R CrB is caused by extinction of the radiation of the star in an infinitely expanding elementary dust cloud. By varying the mass of the dust component, a set of elementary light curves is obtained whose superposition can be used to approximate the real curves. The calculated light curve is compared with the observed minimum of 1972.

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