Cyclical Spectral and Photometric Variations of the Apparently Single Wolf-Rayet Star WR 134

Details Cyclical Spectral and Photometric Variations of the Apparently Single Wolf-Rayet Star WR 134 Cyclical Spectral and Photometric Variations of the Apparently Single Wolf-Rayet Star WR 134

Oct 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998ap%26ss.260..173m&link_type=abstract

Astrophysics and Space Science, v. 260, Issue 1/2, p. 173-176 (1998).

Astronomy and Astrophysics

Astrophysics

Scientific paper

Evidence is presented for the existence of a 2.3 day periodicity in the
line-profile changes of the apparently singleWolf-Rayet star WR 134.
This cyclical variability may be induced either by the presence of an
orbiting collapsed companion, or by the rotational modulation of a
largely inhomogeneous outflow.

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