Interpretation of photometric observations of R Coronae Borealis - Approximation tables

Details Interpretation of photometric observations of R Coronae Borealis - Approximation tables Interpretation of photometric observations of R Coronae Borealis - Approximation tables

Apr 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993azh....70..327p&link_type=abstract

Astronomicheskij Zhurnal (ISSN 0004-6299), vol. 70, no. 2, p. 327-338.

Statistics

Computation

3

Computational Astrophysics, Light Curve, R Coronae Borealis Stars, Stellar Spectrophotometry, Approximation, Stellar Models, Tables (Data)

Scientific paper

A set of light curves is calculated in accordance with a previously described eruptive model of the brightness variability of the R CrB-type stars; this set makes it possible to approximate single and complex brightness fadings of different depth and duration. The approximation tables make it possible to determine, on the basis of the observed light curve, the minimum mass of the cloud dust component and the projected distance of the cloud from the star. This method is suitable for describing the photometric behavior of other R CrB-type stars after slight additions that take the individual features of a specific star into account.

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