Light-curve modeling of the binary star AK Herculis

Details Light-curve modeling of the binary star AK Herculis Light-curve modeling of the binary star AK Herculis

Oct 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985pasp...97.1005n&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 97, Oct. 1985, p. 1005-1010.

Astronomy and Astrophysics

Astronomy

4

Eclipsing Binary Stars, Light Curve, Stellar Spectrophotometry, Electrophotometry

Scientific paper

Light-curve modeling of the W UMa class of binary-star systems is now done by a number of authors. A solution of the photoelectric R and I observations of AK Her by Bookmyer and Kaitchuck (1979) are presented and compared to four different analyses of three different sets of photoelectric B and V observations. The set of parameters solved for in each case varies as do the limits of the numerical values of some of the parameters, most notably the reflection albedo. The results do differ but even though the methods are divergent, the results are fairly consistent.

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