Light Curve Analysis of GSC 2750-0054 and GSC 03208-02644
arXiv:1602.04100 · doi:10.1016/j.newast.2016.05.007
Abstract
We present the first photometric analysis for the newly discovered eclipsing binary systems of Algole-type GSC 2750-0054 and GSC 03208-02644. Our analysis was carried out by means of the most recent version of Wilson Devinney (WD) code, which applies the model atmosphere by Kurucz (1993) with prescription in pass band for the radiative treatment. The accepted light curve solutions reveal absolute physical parameters and the spectral classifications for the components are adopted. Distance to each system was calculated based on the parameters of the accepted photometric solutions. Comparison with the evolutionary models are presented.
arXiv comment11 pages, 6 figures, Submitted to New Astronomy
References in corpus (5)
- Evolutionary tracks and isochrones for low- and intermediate-mass stars: from 0.15 to 7 M_sun, and from Z=0.0004 to 0.03
- Main-Sequence Effective Temperatures from a Revised Mass-Luminosity Relation Based on Accurate Properties
- Detached double-lined eclipsing binaries as critical tests of stellar evolution : Age and metallicity determinations from the HR diagram
- The Catalogue of Stellar Parameters from the Detached Double-Lined Eclipsing Binaries in the Milky Way
- First Orbital Solution and Evolutionary State for the Newly Discovered Eclipsing Binaries USNO-B1.0 1091-0130715 and GSC-03449-0680