Analysis of some photometric observations of Gamma2 Velorum obtained from the South Pole

Details Analysis of some photometric observations of Gamma2 Velorum obtained from the South Pole Analysis of some photometric observations of Gamma2 Velorum obtained from the South Pole

Dec 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988pasp..100.1544t&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 100, Dec. 1988, p. 1544-1548. Research supported by the

Other

8

Binary Stars, Line Spectra, Stellar Spectrophotometry, Wolf-Rayet Stars, Astronomical Photometry, Emission Spectra, Helium, Power Spectra

Scientific paper

The authors discuss the results and analysis of 16 hours of continuous photometry of γ2Vel. Indication of a 1.26-hour period of variability in the He II and C III emission lines at 4686 Å and 5696 Å, respectively, is presented. Although such a period has not been reported by other investigators, recent theoretical studies indicate that such a period may have certain theoretical implications.

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