Changes in AM Herculis during maximum and minimum states

Details Changes in AM Herculis during maximum and minimum states Changes in AM Herculis during maximum and minimum states

Feb 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978pasp...90...61s&link_type=abstract

Astronomical Society of the Pacific, Publications, vol. 90, Feb.-Mar. 1978, p. 61-70.

Astronomy and Astrophysics

Astronomy

16

Binary Stars, Light Curve, Variable Stars, X Ray Stars, Dwarf Stars, Fourier Analysis, Novae, Radial Velocity, Stellar Magnitude, Stellar Mass Accretion, Stellar Models, Ubv Spectra

Scientific paper

Fourier analysis of visual light curves of AM Herculis in U, B, V, and R (which included the minimum and maximum states) made over a period of four days, indicates repetition of periods on minute time scales. A binary model is also presented which accounts for the data with blocked regions, and seeks to systematize changes from cycle to cycle as well as changes occurring over a period of seven months. Cataclysmic variables are employed to compare the two systems, and major differences are revealed.

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