Photometric investigation of AM Herculis

Details Photometric investigation of AM Herculis Photometric investigation of AM Herculis

Dec 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985kfnt....1...43s&link_type=abstract

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 1, Nov.-Dec. 1985, p. 43-46. In Russian.

Physics

1

Binary Stars, Brightness Distribution, Light Curve, Spectral Energy Distribution, Stellar Orbits, Stellar Spectrophotometry, X Ray Binaries

Scientific paper

Orbital light curves obtained during 1979-1983 for different states of the mean brightness of AM Her are analyzed. The dependence of the amplitude of these curves on the mean brightness was obtained; the highest amplitude was observed at the beginning and end of the 'active' state. The variation of mean brightness during the period of observations was found to have a semiregular character with alternation of wide (500-600d) and narrow (350-400d) waves, with an average cycle of 900d.

Affiliated with

Also associated with

No associations

Rating

Photometric investigation of AM Herculis 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 Photometric investigation of AM Herculis, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Photometric investigation of AM Herculis will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1162603