A Possible Secondary Minimum of the Long Period Eclipsing Binary OW Gem (NSV 3005)

Details A Possible Secondary Minimum of the Long Period Eclipsing Binary OW Gem (NSV 3005) A Possible Secondary Minimum of the Long Period Eclipsing Binary OW Gem (NSV 3005)

Jun 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989javso..18....7w&link_type=abstract

The Journal of the American Association of Variable Star Observers. vol. 18, no. 1, p. 7-9

Computer Science

9

Ow Gem

Scientific paper

Photoelectric photometry of the 1258-day eclipsing binary OW Gem = NSV 3005 during the 1988-89 season found the star constant at maximum except for the interval JD 2447531-540, when it was almost 0.1 magnitude fainter. If the observed event was the secondary eclipse, the unseen companion is a large cool star, probably a late-G to early-M giant, and the orbit of the binary system is highly eccentric with secondary minimum occurring at phase 0.23 of the photometric period.

Affiliated with

Also associated with

No associations

Rating

A Possible Secondary Minimum of the Long Period Eclipsing Binary OW Gem (NSV 3005) does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with A Possible Secondary Minimum of the Long Period Eclipsing Binary OW Gem (NSV 3005), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A Possible Secondary Minimum of the Long Period Eclipsing Binary OW Gem (NSV 3005) will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1855345