A spectrophotometric study of the atmospheric eclipses of 32 Cygni

Details A spectrophotometric study of the atmospheric eclipses of 32 Cygni A spectrophotometric study of the atmospheric eclipses of 32 Cygni

Dec 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978phdt........12m&link_type=abstract

Ph.D. Thesis Indiana Univ., Bloomington.

Physics

2

Cygnus Constellation, Eclipses, Eclipsing Binary Stars, Spectrophotometry, Atmospheric Models, Parameterization, Stellar Atmospheres, Supergiant Stars, Wavelengths

Scientific paper

Thirty-two (32) Cygni is one of a small group of eclipsing binaries commonly referred to as Zeta Aurigae systems in which a relatively small main sequence B star is periodically eclipsed by the extended atmosphere of a K type supergaint. A physical model of the system was obtained in terms of masses, sizes, and orbital parameters of the components as well as to determine the structure of the supergaint atmosphere that produces the gradual, wavelength dependent, extinction of light from the B component.

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