UBV photometry of AW Pegasi

Details UBV photometry of AW Pegasi UBV photometry of AW Pegasi

Mar 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992ap%26ss.189..309d&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 189, no. 2, March 1992, p. 309-325. Research supported by Ankara Universit

Astronomy and Astrophysics

Astrophysics

3

Eclipsing Binary Stars, Stellar Spectrophotometry, Ubv Spectra, Light Curve, Stellar Color

Scientific paper

New UBV observations of the classical Algol system AW Peg were presented. The photometric minima times were collected and used together with the new determinations in a period study. No sign of any period change was found from observations covering more than sixty years. The B and V light curves are analyzed by means of the Wilson-Devinney approach. It was verified that the system is semi-detached with a Roche lobe filling secondary.

Affiliated with

Also associated with

No associations

Rating

UBV photometry of AW 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 UBV photometry of AW Pegasi, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and UBV photometry of AW Pegasi will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1215041