UBV observations of short-period close binary V392 Orionis

Details UBV observations of short-period close binary V392 Orionis UBV observations of short-period close binary V392 Orionis

Feb 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988ap%26ss.141...21l&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 141, no. 1, Feb. 1988, p. 21-25. Research supported by the Chinese State E

Astronomy and Astrophysics

Astrophysics

1

Eclipsing Binary Stars, Light Curve, Stellar Spectrophotometry, Ubv Spectra, A Stars, Algol, Tables (Data)

Scientific paper

The eclipsing binary V392 Ori was observed photoelectrically, from November 1984 to January 1985, in UBV 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 minima 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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