Brightness distribution over the disk of MU Geminorum, derived from lunar occultations

Details Brightness distribution over the disk of MU Geminorum, derived from lunar occultations Brightness distribution over the disk of MU Geminorum, derived from lunar occultations

Oct 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984azh....61..944b&link_type=abstract

(Astronomicheskii Zhurnal, vol. 61, Sept.-Oct. 1984, p. 944-955) Soviet Astronomy (ISSN 0038-5301), vol. 28, Sept.-Oct. 1984, p.

Astronomy and Astrophysics

Astronomy

2

Brightness Distribution, Lunar Occultation, Red Giant Stars, Stellar Atmospheres, Angular Velocity, Astronomical Photometry, Diameters, Stellar Models, Stellar Structure

Scientific paper

The influence of the brightness distribution across the disk of a star on its lunar occultation curve is investigated. A method is described which allows to find the radial brightness distribution across a stellar disk directly from the occultation curve. From an analysis of the average occultation curve the brightness distribution across the disk of the red giant μ Gem is derived. The results are compared with the calculations of extended atmosphere models for late-type stars.

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