First frequency analysis for three new members of the group of eclipsing binaries with a pulsating component

被引：7

作者：

Liakos, Alexios ^{[1
]}

Cagas, Pavel ^{[2
]}

机构：

[1] Natl Observ Athens, Inst Astron Astrophys Space Applicat & Remote Sen, Athens 15236, Greece

[2] BSObservatory, Zlin 76001, Czech Republic

来源：

ASTROPHYSICS AND SPACE SCIENCE | 2014年 / 353卷 / 02期

基金：

美国国家科学基金会; 美国国家航空航天局;

关键词：

Methods: data analysis; Methods: observational; Stars: binaries: eclipsing; Stars: fundamental parameters; Stars: variables: delta Scuti; Stars: evolution; Stars:; individual:; V729; Aql; USNO-A2.0; 0975-17281677; 1200-03937339; STAR LIGHT; CATALOG;

D O I：

10.1007/s10509-014-2042-4

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present the first light curves and pulsation analysis results for V729 Aql and two newly discovered eclipsing binaries, namely USNO-A2.0 0975-17281677 and USNO-A2.0 1200-03937339. Frequency search was applied on the residuals of their light curves and the results showed that their primary components pulsate in multiperiodic modes and lie well inside the frequency and temperature range of delta Scuti stars. Moreover, for USNO-A2.0 1200-03937339 two frequencies inside the gamma Dor frequency range were also detected, but their origin is discussed. The photometric models of USNO-A2.0 1200-03937339 and V729 Aql are also presented, while their absolute parameters as well as the evolutionary status of their components were roughly estimated.

引用

页码：559 / 566

页数：8