Inverse photometric problem for spotted stars

Details Inverse photometric problem for spotted stars Inverse photometric problem for spotted stars

Nov 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987ap%26ss.138..141k&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 138, no. 1, Nov. 1987, p. 141-145.

Statistics

Computation

6

Light Curve, Line Of Sight, Stellar Rotation, Stellar Temperature, Computational Astrophysics, High Temperature, Stellar Spectrophotometry

Scientific paper

On the basis of the analytical solution of the direct photometric problem for spotted stars a solution of the corresponding inverse problem is obtained. Expressions are given for determination of the location, size, and temperature of the spot and of the inclination of the rotational axis of the spotted star with regard to the line-of-sight.

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