http://arxiv.org/abs/1712.03540
We observed the recently discovered eccentric eclipsing binary GSC 04052-01378 in order to improve the light curve parameters and to find further evidence of its probable high eccentricity and of apsidal motion. Furthermore, we propose a basic stellar model that fits very well the observations of our dataset and where the eccentricity is found to be e = 0.538(6), which corresponds to an high value among this group of binaries.
R. Furgoni and G. Billings
Tue, 12 Dec 17
7/78
Comments: 7 pages, 6 figures, 5 tables in The Journal of the American Association of Variable Star Observers, vol.45 n.2, 2017