A spectrophotometric study of GG Cassiopeiae

Details A spectrophotometric study of GG Cassiopeiae A spectrophotometric study of GG Cassiopeiae

Jan 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989ap%26ss.151..335c&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 151, no. 2, Jan. 1989, p. 335-341.

Astronomy and Astrophysics

Astrophysics

Cassiopeia Constellation, Eclipsing Binary Stars, Stellar Spectrophotometry, Atmospheric Models, B Stars, Color-Color Diagram, Continuous Spectra, K Stars, Visible Spectrum

Scientific paper

The continuum energy distributions of the totally eclipsing binary
system GG Cas at phases 0.903 P and 0.003 P in the wavelength range
3200-7600 A have been presented and discussed. The flux of the continuum
of the secondary star seems to dominate longward of 4500 A. The spectral
types of the systemic components are found to be B4 + KO.

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