Photometric Study of BD+37DEG2536 Contact System

Details Photometric Study of BD+37DEG2536 Contact System Photometric Study of BD+37DEG2536 Contact System

Sep 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988acasn..29...16l&link_type=abstract

Acta Astronomica Sinica, Vol.29:1, P. 16, 1988

Astronomy and Astrophysics

Astronomy

4

Scientific paper

The photoelectric observations of BD +37°2356 on UBV bands were made using the photometer attached to the 0.91 m telescope at McDonald Observatory in March and May 1984. The UBV light curves were analyzed by the Wilson-Devinney method, according to two normal models without or with spots. BD +37°2356 was found to be a contact system, having a mass ratio of 0.87 and the orbital inclination of 69°. The polar temperatures of two components are almost equal. The authors improved photometric solutions are different from that of Zhukov. The absolute parameters of BD +37°2356 binary were found.

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