UBV observations of short-period close binary V392 Orionis

descriptionPublicationkeyboard_double_arrow_right Article 01 Jan 1988 English Publisher:Springer Science and Business Media LLCJournal:Astrophysics and Space Science, volume 141, pages 21-25 (issn: 0004-640X, eissn: 1572-946X,

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Authors: Xue-Fu Liu; Hui-Song Tan; Kam-Ching Leung;

doi: 10.1007/bf00641912

UBV observations of short-period close binary V392 Orionis

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Abstract

The eclipsing binary V392 Ori was observed photoelectrically, from November 1984 to January 1985, inUBV bands using the P34B photometer attached to the 0.91 m reflector at the McDonald Observatory. Four-hundred eighty-six observations in each band were obtained. Six primary and 4 secondary minimum were observed during this period. The light curves show a typical Beta Lyrae-type variation instead of an Algol-type light curve reported earlier.

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