High-speed photometry of the WO Wolf-Rayet star ST3

Details High-speed photometry of the WO Wolf-Rayet star ST3 High-speed photometry of the WO Wolf-Rayet star ST3

Jul 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986a%26a...162..114l&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 162, no. 1-2, July 1986, p. 114-116. NSERC-supported research.

Astronomy and Astrophysics

Astrophysics

8

Stellar Spectrophotometry, Wolf-Rayet Stars, Amplitudes, Fast Fourier Transformations, Frequency Response, High Speed

Scientific paper

Rapid photometry through Strömgren b and Johnson B filters is reported for the Oxygen-sequence Wolf-Rayet star Stephenson 3. A Fast Fourier Transform analysis does not reveal any significant periodic signal above the noise (≡0m.001) in the range 1 - 70 min. This result may have important implications relative to the basic question of pulsations of Wolf-Rayet stars.

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