Spectropolarimetric observations of WR 137

Details Spectropolarimetric observations of WR 137 Spectropolarimetric observations of WR 137

Nov 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994ap%26ss.221..365h&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 221, no. 1-2, p. 365-367

Astronomy and Astrophysics

Astronomy

B Stars, Infrared Astronomy, O Stars, Spectrum Analysis, Stellar Evolution, Stellar Physics, Stellar Winds, Wolf-Rayet Stars, Astronomical Polarimetry, Astronomical Spectroscopy, Cosmic Dust, Data Reduction, Infrared Spectra, Line Spectra, Polarization, Signal To Noise Ratios

Scientific paper

We present high signal-to-noise spectropolarimetry of the WC7+OB star WR
137 (HD 192641) covering the spectral range from 3600 A to 1.1 microns.
The polarization spectrum shows unambiguous evidence for an intrinsic
polarization vector.

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