Noneclipse periodic optical variability of V 471 Tau

Details Noneclipse periodic optical variability of V 471 Tau Noneclipse periodic optical variability of V 471 Tau

Feb 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988azh....65..194a&link_type=abstract

Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 65, Jan.-Feb. 1988, p. 194-199. In Russian.

Other

Eclipsing Binary Stars, Light Curve, Periodic Variations, Visible Spectrum, White Dwarf Stars, Ultraviolet Filters, X Ray Spectra

Scientific paper

The results of the study of short-timescale optical light variability of V471 Tau in ultraviolet filters are given. The timescales of the short-period variations are close to the period of X-ray pulses and are P ≡ 13 min near the white dwarf's eclipse and ≡9.2 min in other parts of the orbital light curve. The variations' amplitude attains ≡4 - 5%. There is no regular variability in the moment of the white dwarf's eclipse.

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