Spectral investigation of the eclipsing binary star V 367 Cygni

Details Spectral investigation of the eclipsing binary star V 367 Cygni Spectral investigation of the eclipsing binary star V 367 Cygni

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985azh....62..744k&link_type=abstract

(Astronomicheskii Zhurnal, vol. 62, July-Aug. 1985, p. 744-750) Soviet Astronomy (ISSN 0038-5301), vol. 29, July-Aug. 1985, p. 4

Astronomy and Astrophysics

Astronomy

1

Eclipsing Binary Stars, Stellar Spectra, Line Spectra, Spectral Line Width, Spectrum Analysis, Stellar Composition, Stellar Envelopes, Stellar Temperature

Scientific paper

An analysis of the line spectrum of the binary star V367 Cygni has been carried out from diffraction spectrograms. Physical parameters of the star's shell have been determined by the curve-of-growth method, the results obtained have been compared with those of other authors. The authors have obtained a general agreement of the results, increased values of electron pressure apparently in the gaseous flux, and chemical composition slightly different (for titanium) from that of the sun.

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