Photometry of an active Algol-type binary HP Aur

Details Photometry of an active Algol-type binary HP Aur Photometry of an active Algol-type binary HP Aur

Apr 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989ap%26ss.154....1x&link_type=abstract

Astrophysics and Space Science, Volume 154, Issue 1, pp.1-6

Astronomy and Astrophysics

Astrophysics

Scientific paper

The short period Algol-type binary HP Aur has been studied on the basis ofUBV photometric observations. Its colour indexes were found to be (U-B)=0.14, (B-V)=0.70, and light curves show non-symmetrical and obvious photometric disturbances. Autoregressive spectral analysis and harmonic analysis for its light variations were made. The results indicate its brightness variations have the multiplet quasi-periods and low amplitudes. Its photometric solutions have been obtained using the Wilson-Devinney method. Its mass ratio is 0.5631, orbital inclination is 85.0 and it is a detached system. Its basic model has been discussed briefly.

Affiliated with

Also associated with

No associations

Rating

Photometry of an active Algol-type binary HP Aur 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 Photometry of an active Algol-type binary HP Aur, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Photometry of an active Algol-type binary HP Aur will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1735310