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Kondo, Y. ; Drechsel, H. ; Mccluskey, G. E., Jr. ; [et al.]

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Publication Date: 2011-08-18

Description: The interacting close binary system UW CMa has been observed, in the wavelength range from 1161 to 1188 A, continuously during a complete orbital cycle in 1979 with the Copernicus (OAO-3) U2 spectrometer. The C III multiplet at 1175 A, observed as a P Cygni feature, exhbits a clear dependence on the orbital phase of the binary; the radial velocity variation of this feature lags behind that of the O7 primary component by 0.1 orbital phase, which agrees with the anticipations in an earlier study by the same authors. The radiation-driven matter, flowing out of the binary, originates in the primary component.

Keywords: ASTRONOMY

Type: Astronomy and Astrophysics; 94; 2, Fe; Feb. 198

Format: text

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