TU Horologii - an ellipsoidal variable

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Eclipsing Binary Stars, Stellar Spectra, Ubv Spectra, Harmonic Analysis, Light Curve

Scientific paper

From UBV observations, TU Hor is found to be an ellipsoidal variable (V
magnitude of 5.925 to 6.025) with a period of 0.935984 day. Analysis of
the light variation indicates abnormal reflection behavior in close
binary systems. Spectroscopic observations yield an orbital inclination
of about 35 deg.

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