Spectroscopic and Photometric Solution of the Binary System BD+14 d 5016

Details Spectroscopic and Photometric Solution of the Binary System BD+14 d 5016 Spectroscopic and Photometric Solution of the Binary System BD+14 d 5016

Apr 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003ibvs.5400....1m&link_type=abstract

Information Bulletin on Variable Stars, 5400, 1.

Computer Science

5

Ew, Orbital Solutions

Scientific paper

We present preliminary solution of the eclipsing binary star BD+14 5016.
The obtained model indicates that the investigated star is an A-type W
UMa system with a hot spot located on the surface of the more massive
component. The system is in a large degree of overcontact of about 54
percent.

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