تقرير
NSVS07394765: A new low-mass eclipsing binary below 0.6 M_sun
| العنوان: | NSVS07394765: A new low-mass eclipsing binary below 0.6 M_sun |
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| المؤلفون: | Çakirli, Ö. |
| سنة النشر: | 2013 |
| المجموعة: | Astrophysics |
| مصطلحات موضوعية: | Astrophysics - Solar and Stellar Astrophysics |
| الوصف: | The multi-color photometric and spectroscopic (based on observations obtained with the T{\"U}B{\.I}TAK National Observatory 1.5-meter telescope, which is owned and operated by the T{\"U}B{\.I}TAK) observations of the newly discovered eclipsing binary NSVS 07394765 were obtained. The resultant light and radial velocities were analysed and the global parameters of the system: T$_{1}$=3 300 K; T$_{2}$=3 106 K; M$_1$=0.36 M$_{\odot}$; M$_2$=0.18 M$_{\odot}$; R$_1$=0.46 R$_{\odot}$; R$_2$=0.50 R$_{\odot}$; L$_{1}$=0.030 L$_{\odot}$; L$_2$=0.026 L$_{\odot}$; $i=89.2{^\circ}$; $a=5.97$ R$_{\odot}$; $d=28$ pc. The chromospheric activity of its components is revealed by strong emission in the H$\alpha$ line and observed flares. Empirical relations for mass-radius and mass-temperature are derived on the basis of the parameters of known binaries with low-mass dM components. Comment: Accepted in New Astronomy, 25 pages, 7 figures. arXiv admin note: text overlap with arXiv:0909.1921, arXiv:1210.8133, arXiv:1209.0271; and with arXiv:1005.0260 by other authors |
| نوع الوثيقة: | Working Paper |
| DOI: | 10.1016/j.newast.2012.12.001 |
| URL الوصول: | http://arxiv.org/abs/1301.0423 |
| رقم الأكسشن: | edsarx.1301.0423 |
| قاعدة البيانات: | arXiv |
| DOI: | 10.1016/j.newast.2012.12.001 |
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