Dynamical parallax, physical parameters, and evolutionary status of the components of the bright eclipsing binary alpha Draconis
Özet
Aims. Both components of the bright eclipsing binary a Dra have been resolved using long baseline interferometry and the secondary component has been shown to contribute approximately 15% of the total flux; however, a spectroscopic detection of the companion star has so far been unsuccessful. We aim for a firm spectroscopic detection of the secondary component of alpha Dra using state-of-the-art spectroscopic analysis methods for very high-quality spectroscopic observations. This will allow the determination of fundamental and atmospheric properties of the components in the system with high precision and accuracy.
Anahtar kelimeler
Atıf için künye
Pavlovski, K., Hummel, C. A., Tkachenko, A., Dervişoğlu, A., Kayhan, C., Zavala, R. T., Hutter, D. J., Tycner, C., ŞAHİN, T., Audenaert, J., Baeyens, R., Bodensteiner, J., Bowman, D. M., Gebruers, S., Jannsen, N. E., & Mombarg, J. S. G. (2022). Dynamical parallax, physical parameters, and evolutionary status of the components of the bright eclipsing binary alpha Draconis. ASTRONOMY & ASTROPHYSICS, 658. https://doi.org/10.1051/0004-6361/202142292
BibTeX
@article{pavlovski2022-79915,
author = {Pavlovski, K. and Hummel, C. A. and Tkachenko, A. and Dervişoğlu, Ahmet and Kayhan, C. and Zavala, R. T. and Hutter, D. J. and Tycner, C. and ŞAHİN, TİMUR and Audenaert, J. and Baeyens, R. and Bodensteiner, J. and Bowman, D. M. and Gebruers, S. and Jannsen, N. E. and Mombarg, J. S. G.},
title = {Dynamical parallax, physical parameters, and evolutionary status of the components of the bright eclipsing binary alpha Draconis},
journal = {ASTRONOMY & ASTROPHYSICS},
year = {2022},
volume = {658},
issn = {0004-6361},
doi = {10.1051/0004-6361/202142292},
url = {https://akademik.atauni.edu.tr/yayinlar/79915-dynamical-parallax-physical-parameters-and-evolutionary-status-of-the-components}
}