Properties of the main-sequence eclipsing binary UZ Draconis

Details Properties of the main-sequence eclipsing binary UZ Draconis Properties of the main-sequence eclipsing binary UZ Draconis

Mar 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989aj.....97..822l&link_type=abstract

Astronomical Journal (ISSN 0004-6256), vol. 97, March 1989, p. 822-835. Research supported by NSF.

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3

Eclipsing Binary Stars, Main Sequence Stars, Stellar Evolution, Stellar Spectrophotometry, Light Curve, Line Spectra, Radial Velocity, Spectral Line Width

Scientific paper

The fundamental properties of the main-sequence binary, UZ Dra, are determined from observational data. Photoelectric radial-velocity measurements (Imbert, 1986), spectroscopic data obtained with solid-state array detectors, and B,V photoelectric light curves of the binary are examined. The properties of the stars in the binary are presented and compared with those of other F-type main-sequence binaries listed by Popper (1980).

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