Luminosity dependence of the AM Herculis light curve

Details Luminosity dependence of the AM Herculis light curve Luminosity dependence of the AM Herculis light curve

Apr 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985pazh...11..203a&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 11, Mar. 1985, p. 203, 207) Soviet Astronomy Letters (ISSN 0360-0327), vol. 11, Mar.-Ap

Astronomy and Astrophysics

Astronomy

3

Light Curve, Stellar Luminosity, X Ray Binaries, Astronomical Photometry, Least Squares Method

Scientific paper

The luminosity dependence of the orbital light curve of AM Her in its active state is investigated on the basis of yellow-band photometry in 1978-1979. When the system is at mean magnitude 12.4-13.1 m, the amplitude of the intensity variation is nearly independent of luminosity; but as the object brightens further, the primary maximum becomes more prominent and the light curve comes to resemble the nonflare curve of U Gem.

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