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Title:
An eight-year spectroscopic orbit for the WC7 + O4 Wolf-Rayet binary HD 193793 - Toward solving the mystery of the infrared outbursts
Authors:
Moffat, Anthony F. J.; Lamontagne, Robert; Williams, Peredur M.; Horn, Jiri; Seggewiss, Wilhelm
Affiliation:
AA(Montreal, Universite, Montreal; Observatoire Astronomique du Mont Megantic, Montreal, Notre-Dame-des-Bois, Canada), AB(Montreal, Universite, Montreal; Observatoire Astronomique du Mont Megantic, Montreal, Notre-Dame-des-Bois, Canada), AC(Royal Observatory, Edinburgh, Scotland), AD(Astronomicka Observator, Ondrejov, Czechoslovakia), AE(Observatorium Hoher List, Daun, Germany)
Publication:
Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 312, Jan. 15, 1987, p. 807-811. NSERC-supported research. (ApJ Homepage)
Publication Date:
01/1987
Category:
Astrophysics
Origin:
STI
NASA/STI Keywords:
Binary Stars, Infrared Spectra, Radial Velocity, Stellar Orbits, Stellar Spectrophotometry, Wolf-Rayet Stars, Absorption Spectra, Emission Spectra, Stellar Mass
DOI:
10.1086/164925
Bibliographic Code:
1987ApJ...312..807M

Abstract

Some 60 yr of spectroscopic radial velocity data combined from many different sources lead to a 7.9 yr period for this once enigmatic system. The masses and mass ratio derived are compatible with other close systems containing stars of similar type. It is no coincidence that infrared flux enhancement occurs just before periastron passage in the e = 0.7 orbit.

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