Angular diameters of stars determined from an analysis of photoelectric observations of lunar occultations

Details Angular diameters of stars determined from an analysis of photoelectric observations of lunar occultations Angular diameters of stars determined from an analysis of photoelectric observations of lunar occultations

Feb 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990pazh...16..160k&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 16, Feb. 1990, p. 160-162. In Russian. In Russian. In Russian.

Astronomy and Astrophysics

Astronomy

1

Lunar Occultation, Size Determination, Stellar Structure, Diameters, Electrophotometers

Scientific paper

Angular diameters are calculated for two stars on the basis of the lunar
occultation technique. For SAO 076532, D = 0.0025 arcsec for beta = 1
and D = 0.0022 arcsec for beta = 0, where beta is the darkening
coefficient. For SAO 076585, D = 0.0021 arcsec for beta = 0 and D =
0.0023 arcsec for beta = 1.

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