Light variations of spotted stars - Second approximation

Details Light variations of spotted stars - Second approximation Light variations of spotted stars - Second approximation

May 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989ap%26ss.155..203k&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 155, no. 2, May 1989, p. 203-207. Research supported by the Bulgarian Comm

Astronomy and Astrophysics

Astrophysics

5

Giant Stars, Light Curve, Limb Darkening, Starspots, Stellar Activity, Astronomical Photometry, F Stars, K Stars, Stellar Spectra

Scientific paper

The light variations of spotted giants are analyzed, using a quadratic
limb-darkening law. The results may be used for solving the inverse
photometric problem for spotted late FK Com-type giants and may be
applied directly for different stellar configurations with different
spot numbers, sizes, and locations.

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