Two colour photometry and analysis of the eclipsing binary at Pegasi

Details Two colour photometry and analysis of the eclipsing binary at Pegasi Two colour photometry and analysis of the eclipsing binary at Pegasi

Aug 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993ap%26ss.206..259g&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 206, no. 2, p. 259-274

Physics

Eclipsing Binary Stars, Light Curve, Stellar Physics, Astronomical Photometry, Color-Color Diagram, Orbital Mechanics, Stellar Composition

Scientific paper

Two-color photoelectric observations of the eclipsing binary AT Pegasi have been carried out at the Ege University Observatory. The light curves were analyzed with the methods of Wood and Wilson-Devinney. It is found that the period of the system is decreasing. The system was found to be an Algol type semi-detached binary. The absolute elements of the system are also deduced.

Affiliated with

Also associated with

No associations

Rating

Two colour photometry and analysis of the eclipsing binary at Pegasi 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 Two colour photometry and analysis of the eclipsing binary at Pegasi, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Two colour photometry and analysis of the eclipsing binary at Pegasi will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1490975