Further results on the line-profile variability of WR 134

Details Further results on the line-profile variability of WR 134 Further results on the line-profile variability of WR 134

Nov 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994ap%26ss.221..181g&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 221, no. 1-2, p. 181-188

Physics

4

Cygnus Constellation, Spectrum Analysis, Stellar Physics, Stellar Winds, Variability, Wolf-Rayet Stars, Brightness, Line Spectra, Time Series Analysis

Scientific paper

We discuss a few conclusions previously derived from the analysis of the
line-profile variability of the Wolf-Rayet star WR 134, some details are
made more explicit. In addition, we present a new set of data and
briefly comment on recent results deduced from its analysis.

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