A radial velocity and photometric study of the eclipsing binary RT Andromedae

Details A radial velocity and photometric study of the eclipsing binary RT Andromedae A radial velocity and photometric study of the eclipsing binary RT Andromedae

Jun 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992acaps..12...25w&link_type=abstract

(Acta Astrophysica Sinica, vol. 12, no. 1, 1992, p. 25-33) Chinese Astronomy and Astrophysics (ISSN 0275-1062), vol. 16, no. 2,

Astronomy and Astrophysics

Astrophysics

1

Astronomical Photometry, Astronomical Spectroscopy, Eclipsing Binary Stars, Radial Velocity, Stellar Spectra, Andromeda Constellation, Light Curve, Main Sequence Stars, Roche Limit, Stellar Magnitude, Stellar Mass

Scientific paper

Radial velocity observations of the eclipsing binary RT Andromedae performed in 1984-85 are presented. RT Andromedae is a detached system comprising two main sequence stars both showing a slight departure from the ZAMS. Attention is focused on determining the radial velocity of the companion star for a determination of the spectroscopic orbit using new radial velocity observations.

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