Temperature distribution in the atmosphere of the Wolf-Rayet component of V444 Cygni, based on infrared data

Details Temperature distribution in the atmosphere of the Wolf-Rayet component of V444 Cygni, based on infrared data Temperature distribution in the atmosphere of the Wolf-Rayet component of V444 Cygni, based on infrared data

Dec 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982sval....8..391b&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 8, Dec. 1982, p. 725-728) Soviet Astronomy Letters (ISSN 0360-0327), vol. 8, Nov.-Dec.

Astronomy and Astrophysics

Astronomy

1

Eclipsing Binary Stars, Infrared Spectra, Stellar Atmospheres, Temperature Distribution, Wolf-Rayet Stars, Atmospheric Temperature, Brightness Distribution, Temperature Profiles

Scientific paper

An analysis of the infrared brightness distribution across the disk of
the Wolf-Rayet star in the V444 Cyg eclipsing binary system yields
source functions and temperature profiles in its atmosphere. The results
are compared against model calculations for extended atmospheres.

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