Existence of a short period (3.5-4 hours) in the photometric variability of WR66.

Details Existence of a short period (3.5-4 hours) in the photometric variability of WR66. Existence of a short period (3.5-4 hours) in the photometric variability of WR66.

Feb 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996a%26a...306..783r&link_type=abstract

Astronomy and Astrophysics, v.306, p.783

Astronomy and Astrophysics

Astrophysics

9

Stars: Individual: Wr66, Stars: Wolf-Rayet, Stars: Mass-Loss, Stars: Variables

Scientific paper

We report here on an independent detection of a short period (~4hours) in the photometric variations of WR66, thus confirming in broad terms the discovery by Antokhin et al.. In addition, we present the first spectroscopic variability analysis for this star. A few peculiarities of the spectrum of WR66 are also discussed. Finally, we perform a brief examination of different possible origins of the phenomenon.

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