Apsidal motion in the eclipsing binary system HP AUR

Details Apsidal motion in the eclipsing binary system HP AUR Apsidal motion in the eclipsing binary system HP AUR

Mar 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990ap%26ss.165....1k&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 165, no. 1, March 1990, p. 1-7.

Astronomy and Astrophysics

Astrophysics

7

Apsides, Eclipsing Binary Stars, Stellar Motions, Astronomical Observatories, Light Curve, Limb Darkening, Stellar Orbits, Stellar Spectrophotometry

Scientific paper

Multicolor WBVR photoelectric observations of the eclipsing binary HP Aur were carried out. The photometric elements, the absolute parameters and the apsidal motion angular rate of HP Aur based on the comparison of these observations and the observations Meinunger (1980) obtained were presented. The derived value of apsidal motion angle is almost three times smaller than that predicted theoretically.

Affiliated with

Also associated with

No associations

Rating

Apsidal motion in the eclipsing binary system 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 Apsidal motion in the eclipsing binary system HP AUR, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Apsidal motion in the eclipsing binary system HP AUR will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1885855