Contact binaries with components in poor thermal contact. V - BE Cephei

Details Contact binaries with components in poor thermal contact. V - BE Cephei Contact binaries with components in poor thermal contact. V - BE Cephei

Jul 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986pasp...98..662k&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 98, July 1986, p. 662-668.

Astronomy and Astrophysics

Astronomy

16

Cepheus Constellation, Eclipsing Binary Stars, Light Curve, Mass Ratios, B Stars, Roche Limit, Stellar Spectrophotometry, Stellar Temperature

Scientific paper

Photometric observations of BE Cep recently published by Hoffmann (1984) were analyzed using the Wilson-Devinney code. A grid of solutions for several fixed values of the mass ratio was calculated. BE Cep is most probably a contact binary with components in poor thermal contact. The temperature difference between components is about 900 K. The cooler component of the system has a complex surface brightness distribution. Data for 13 contact binaries with components in poor thermal contact are presented.

Affiliated with

Also associated with

No associations

Rating

Contact binaries with components in poor thermal contact. V - BE Cephei 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 Contact binaries with components in poor thermal contact. V - BE Cephei, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Contact binaries with components in poor thermal contact. V - BE Cephei will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1656042