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Long-period Double-lined Eclipsing Binaries: The System V454 Aur with the Secondary Eclipse Caused by the Occultation of the Hotter Componentстатья
- Авторы: Kniazev Alexei Y., Malkov Oleg, Gorda Stanislav, Berdnikov Leonid N., Katkov Ivan Y.
- Журнал: Research in Astronomy and Astrophysics
- Том: 25
- Номер: 2
- Год издания: 2025
- Издательство: IOP Publishing
- Местоположение издательства: [Bristol, UK], England
- Первая страница: 025024
- DOI: 10.1088/1674-4527/adb138
- Аннотация: We present the results of our study of the long-period eclipsing binary star V454 Aur. The results are based on spectroscopic data obtained with the UFES échelle spectrograph and photometric observations from Transiting Exoplanet Survey Satellite (TESS). The derived radial velocity curve is based on 17 spectra obtained between 2021 and 2023, covering all orbital phases of this binary system. The orbital period determined from TESS data, P = 27.019803 ± 0.000003 days, agrees within uncertainties with the period established in previous studies. The model constructed for the TESS photometric light curve achieves a precision of 0.01%. The effective temperatures of both components, as well as the system metallicity, were directly derived from the spectra and are Teff_A = 6250 ± 50 K, Teff_B = 5855 ± 50 K, and [Fe/H] = −0.10 ± 0.08, respectively. Our analysis of the photometric and spectroscopic data allowed us to directly compute the luminosities of the components, L_A = 1.82 Lsun and L_B = 1.07 Lsun, their radii, R_A = 1.15 Rsun and R_B = 1.00 Rsun, and their masses, M_A = 1.137 Msun and M_B = 1.023 Msun, with uncertainties below 1%. Comparison with evolutionary tracks indicates that the system's age is 1.18 ± 0.10 Gyr, and both components are still on the main sequence. The V454 Aur system is particularly interesting due to the partial eclipse of the primary component, which results in the "inversion" of the primary and secondary minima in the photometric light curve.
- Добавил в систему: Катков Иван Юрьевич