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Clumped structure of WR wind derived from IR observations of WR+O binaries: some comments on the light curve solution for V444 Cygni
A. M. CherepashchukVolume:
221
Language:
english
Pages:
11
DOI:
10.1007/bf01091155
Date:
November, 1994
File:
PDF, 994 KB
english, 1994