UBV light curves of V356 Sagittarii

Details UBV light curves of V356 Sagittarii UBV light curves of V356 Sagittarii

Feb 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995pasp..107..132w&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 107, no. 708, P. 132-135

Astronomy and Astrophysics

Astronomy

1

Eclipsing Binary Stars, Light Curve, Ubv Spectra, Stellar Evolution, Stellar Magnitude, Stellar Spectra

Scientific paper

We report here UBV observations of the unusual eclipsing binary V356 Sagittarii from 1973, 1974, and 1975. Although there are phase gaps, light-curve form and absolute level differ only slightly from light curves of 23 years earlier in the phases that are covered. Scatter is anomalously large, as in the earlier observations, and seems to be diagnostic of some intrinsic abnormality.

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