Spectroscopic and photometric detection of interacting processes and their evolution in the eclipsing binary TX UMA

Details Spectroscopic and photometric detection of interacting processes and their evolution in the eclipsing binary TX UMA Spectroscopic and photometric detection of interacting processes and their evolution in the eclipsing binary TX UMA

Dec 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992ap%26ss.198..149k&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 198, no. 1, p. 149-159.

Astronomy and Astrophysics

Astrophysics

Eclipsing Binary Stars, Light Curve, Stellar Evolution, Stellar Spectrophotometry, Radial Velocity, Spectrographs, Stellar Orbits

Scientific paper

Spectroscopic observations of the eclipsing binary TX UMA carried out with D.A.O high-dispersion spectrographs in 1969-70 and at the Ondrejov Observatory in 1972-1980 are summarized. Particular attention is given to the manifestations of interacting processes, the secondary component spectrum in the ever changing line spectra, and orbital period changes obtained by the Skalnate Pleso Observatory.

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