Photoelectric Photometry of OW Geminorum at Phase 0.5

Details Photoelectric Photometry of OW Geminorum at Phase 0.5 Photoelectric Photometry of OW Geminorum at Phase 0.5

Oct 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991javso..20..234w&link_type=abstract

The Journal of the American Association of Variable Star Observers, vol. 20, no. 2, p. 234-235

Physics

1

Scientific paper

Differential V photometry of the 3.45-year eclipsing binary OW Gem near
phase 0.5 shows no indication of a secondary minimum. This result
supports the earlier conclusion that OW Gem is a highly eccentric binary
system with secondary minimum occuring at phase 0.23.

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