The Peculiar Ellipsoidal Variable Tu-Horologii

Details The Peculiar Ellipsoidal Variable Tu-Horologii The Peculiar Ellipsoidal Variable Tu-Horologii

Dec 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982msngr..30...14w&link_type=abstract

The Messenger, No.30, P. 14, 1982

Physics

1

Scientific paper

The peculiar nature of the lightcurve of the sixth magnitude variable A-type star TU Hor (HR 1081 = HD 21981) was first discovered at ESO by H.W. Duerbeck from Bonn Observatory. In subsequent spectroscopic work in collaboration with A. and J. Surdej, Dr. Duerbeck demonstrated conclusively that TU Hor is a close binary star with an orbital period of about 0.936 days.

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