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

Journal Article · · Sov. Astron. Lett. (Engl. Transl.); (United States)
OSTI ID:6120294
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.
Research Organization:
Chernyshevskii University, Saratov, USSR
OSTI ID:
6120294
Journal Information:
Sov. Astron. Lett. (Engl. Transl.); (United States), Journal Name: Sov. Astron. Lett. (Engl. Transl.); (United States) Vol. 8:6; ISSN SALED
Country of Publication:
United States
Language:
English