Four-colour photometry of eclipsing binaries. XXXII - Light curves of V1031 Orionis

Details Four-colour photometry of eclipsing binaries. XXXII - Light curves of V1031 Orionis Four-colour photometry of eclipsing binaries. XXXII - Light curves of V1031 Orionis

Dec 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989a%26as...81..197c&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 81, no. 2, Dec. 1989, p. 197-205. Research supported by SNFO

Astronomy and Astrophysics

Astrophysics

A Stars, Astronomical Photometry, Eclipsing Binary Stars, Light Curve, Triple Stars, Circular Orbits, Ubv Spectra, Variable Stars

Scientific paper

Complete uvby light curves are presented for the bright, southern,
A-type triple system V1031 Orionis which consists of two well-separated
eclipsing components in a circular orbit and a third component at an
angular distance of about 0.16 arcsec. The light curves contain 1280
points in each color, obtained from 1980 to 1983.

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