A spectroscopic study of Epsilon Aurigae

Details A spectroscopic study of Epsilon Aurigae A spectroscopic study of Epsilon Aurigae

Feb 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984ap%26ss..99..269s&link_type=abstract

(International Astronomical Union, Colloquium on Double Stars, Physical Properties and Generic Relations, 80th, Bandung, Indones

Astronomy and Astrophysics

Astrophysics

2

Eclipsing Binary Stars, H Alpha Line, Stellar Spectra, Absorption Spectra, Metallicity, Neutral Gases, Radial Velocity

Scientific paper

Epsilon Aurigae has been observed during ingress and totality between
1982 and 1983 at Okayama. Analyses of profiles of Hα line and of
radial velocities of neutral hydrogen and metals show that the secondary
component has a circumstellar shell consisting of at least three parts.

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