A low-mass model of epsilon Aurigae

Details A low-mass model of epsilon Aurigae A low-mass model of epsilon Aurigae

Mar 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986ap%26ss.120....1t&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 120, no. 1, March 1986, p. 1-7.

Astronomy and Astrophysics

Astrophysics

6

Eclipsing Binary Stars, Stellar Mass, Stellar Models, Stellar Orbits, Accretion Disks, B Stars, Orbital Elements, Supergiant Stars, Variable Stars

Scientific paper

The eclipsing binary system Epsilon Aurigae, containing an unseen component is discussed on the basis of its orbital elements. The masses of the compoents can be approximately 4 solar masses and 1 Solar mass, respectively. it is shown that there is no reason to reject a low-mass model. An opaque elongated eclipsing body is briefly discussed as one of the components which is an accretion disk surrounding a central Main-Sequence star.

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