The new photometric solution and light curve study of the semi-detached binary system ASAS ID 211049-3657.9

被引:1
|
作者
Tanriver, Mehmet [1 ]
机构
[1] Erciyes Univ, Fac Sci, TR-38039 Kayseri, Turkey
关键词
(Stars:) binaries: eclipsing; Stars: late-type; Stars: individual: (ASAS ID 211049-3657.9); Stars: fundamental parameters; SKY AUTOMATED SURVEY; GRAVITY-DARKENING EXPONENTS; ECLIPSING BINARY; VARIABLE-STARS; SOUTHERN-HEMISPHERE; ALGOL BINARIES; CATALOG; PERIOD; QUARTER; GEMINORUM;
D O I
10.1016/j.newast.2014.02.002
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
This work is targeted on the photometric (light curve) analysis of the stars with G2 spectral type. The sun like star (ASAS ID 211049-3657.9) located in the ASAS catalogue was subjected to its photometric solutions and the light curve analysis in V band. The light curve of ASAS ID 211049-3657.9 binary system which belongs to the Southern Hemisphere shows the variation of l Lyr type. The solution of light curve was carried out using the PHOBE code. The photometiic solution reveals a semi-detached configuration with a less-massive component filling its own Roche lobe. The absolute parameters, very close to the astrophysical fundamental values of the sun, are obtained as a result of the solution. A spotted solution for ASAS ID 211049-3657.9 binary system with the Sun-like selected from the solar analogue star list of Tannver (2012, 2013) is conducted. The masses of the primary and secondary components for ASAS ID 211049-3657.9 are M1 = 1.00741 M and M2 = 0.37535 M, respectively. While the radius for the primary was R1 = 1.00097 R, and for the secondary R2 = 1.19107 Ro and the temperature of the primary and secondary are T1 = 5850 K and T2 = 5150 K, respectively. The positions in the HR diagram of the components are also discussed. (C) 2014 Elsevier B.V. All rights reserved.
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页码:20 / 25
页数:6
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