V482 Cygni - an R Coronae Borealis star in a quadruple system

Details V482 Cygni - an R Coronae Borealis star in a quadruple system V482 Cygni - an R Coronae Borealis star in a quadruple system

Mar 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988pasp..100..388g&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 100, March 1988, p. 388-392. Research supported by the

Astronomy and Astrophysics

Astronomy

6

Star Clusters, Stellar Luminosity, Variable Stars, Color-Magnitude Diagram, Stellar Envelopes, Stellar Magnitude, Stellar Temperature

Scientific paper

Observations of the R CrB variable star V482 Cyg, obtained with the University of Rochester 32 x 32 InSb array camera at the NASA IR Telescope Facility on Mauna Kea on August 20, 1984, are reported. The data-reduction and analysis procedures are described in detail, and the results are presented in tables and maps. V482 Cyg is shown to be a member of a quadruple system or perhaps a small obscured cluster. Parameters determined include distance 1.7 kpc, circumstellar-shell temperature 800 K, and absolute magnitude M(V) = -2.8.

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