Spectral analysis of the eclipsing variable V471 Tauri /BD + 16 deg 516/

Details Spectral analysis of the eclipsing variable V471 Tauri /BD + 16 deg 516/ Spectral analysis of the eclipsing variable V471 Tauri /BD + 16 deg 516/

Jun 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981ap%26ss..77..221h&link_type=abstract

Astrophysics and Space Science, vol. 77, no. 1, June 1981, p. 221-233. Research supported by the Scientific and Technical Resea

Astronomy and Astrophysics

Astrophysics

3

Eclipsing Binary Stars, Spectrum Analysis, Stellar Spectra, Stellar Spectrophotometry, Variable Stars, White Dwarf Stars, Calcium, Electrophotometry, Emission Spectra, H Lines, K Lines, Light Curve, Line Spectra, Radial Velocity, Stellar Motions

Scientific paper

Spectroscopic observations are reported of the white-dwarf eclipsing binary V471 Tauri. The behavior of the H and K emission lines of Ca II in relation to the photoelectric observations is investigated, and the existence of a probable correlation between minimum emission line strength and the maximum wave position within the migrating wave is demonstrated.

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