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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Hoffmeister, C.: 1954,Sternwarte Sonneberg Veröffentlichungen, Band II, p. 56.
Meinunger, L.: 1966,Mitteilungen über Veränderliche Sterne herausgegeben von der Sternwarte Sonneberg der Deutschen Akademie der Wissenschaften, Band 3, Heft 6.
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Liu, XF., Tan, HS. & Leung, KC. UBV observations of short-period close binary V392 Orionis. Astrophys Space Sci 141, 21–25 (1988). https://doi.org/10.1007/BF00641912
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DOI: https://doi.org/10.1007/BF00641912