Two New Eclipsing Binaries: V1626 Ori (Brh V38) and GSC 0486-4828 (Brh V64)

Details Two New Eclipsing Binaries: V1626 Ori (Brh V38) and GSC 0486-4828 (Brh V64) Two New Eclipsing Binaries: V1626 Ori (Brh V38) and GSC 0486-4828 (Brh V64)

Nov 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002ibvs.5339....1l&link_type=abstract

Information Bulletin on Variable Stars, 5339, 1.

Physics

2

Eclipsing Binaries, Variable Stars, Photometry

Scientific paper

V1626 Ori is an EA with a period of 1.137793 days containing a mid
F-type main-sequence primary and an oversized early K-type secondary,
which may or may not fill its Roche lobe. GSC 0486-4828 has a period of
9.27850 days and contains two apparently unevolved main-sequence stars
of spectral types late B and early A.

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