Accretion disk in the eclipsing binary AU Mon

Details Accretion disk in the eclipsing binary AU Mon Accretion disk in the eclipsing binary AU Mon

2010-07-22

arxiv.org/abs/1007.3872v2

Astronomy and Astrophysics

Astrophysics

Solar and Stellar Astrophysics

Accepted for publication in MNRAS

Scientific paper

10.1111/j.1365-2966.2010.17310.x

We analyze the CoRoT and V-passband ground-based light curves of the interacting close binary AU Mon, assuming that there is a geometrically and optically thick accretion disk around the hotter and more massive star, as inferred from photometric and spectroscopic characteristics of the binary. Our model fits the observations very well and provides estimates for the orbital elements and physical parameters of the components and of the accretion disk.

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