Photometric Studies of 21 Eclipsing Binaries with Eccentric Orbits

被引：3

作者：

Kozyreva, V. S. ^{[1
]}

Kusakin, A., V ^{[2
]}

Krajci, T. ^{[3
]}

Bogomazov, A., I ^{[1
]}

机构：

[1] Lomonosov Moscow State Univ, Sternberg Astron Inst, Moscow, Russia

[2] Fesenkov Astrophys Inst, Natl Space Agcy Republ Kazakhstan, Alma Ata 050020, Kazakhstan

[3] CBA New Mexico, POB 1351, Cloudcroft, NM 88317 USA

来源：

ASTROPHYSICAL BULLETIN | 2019年 / 74卷 / 04期

关键词：

stars:; binaries:; eclipsing; APSIDAL MOTION; SYSTEM;

D O I：

10.1134/S1990341319040084

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The paper describes a target setting of searching for apsidal motion in 21 eclipsing binaries. We estimate the capability of its determination for the systems of interest in the coming years, as well as present results of observations in 2009-2018, in which the minima of the light curves of these stars have been obtained. The accuracy of orbital period determination of the studied binaries is 10-100 times greater in comparison with the previously available data. For two systems, photometric elements are determined. As a by-product of the study, a close eclipsing binary of the W UMa type was discovered.

引用

页码：424 / 430

页数：7

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