电邮这篇文章 Effect of the Eccentricity of the Planet’s Orbit on the Limb Darkening Coefficients of the Eclipsed Star
- 作者: Bekesov E.V.1,2, Cherepashchuk A.M.1,2
-
隶属关系:
- Sternberg Astronomical Institute
- Moscow State University
- 期: 卷 100, 编号 2 (2023)
- 页面: 173-185
- 栏目: Articles
- URL: https://journals.rcsi.science/0004-6299/article/view/139064
- DOI: https://doi.org/10.31857/S0004629923020020
- EDN: https://elibrary.ru/CIZPKY
- ID: 139064
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详细
It is shown that the introduction of a small orbital eccentricity into the model of a binary system with an exoplanet, which is allowed by errors in determining the radial velocities of the eclipsed star, makes possible to significantly reduce and even eliminate the difference in the wavelength dependences between the observed and theoretical values of the limb darkening coefficients of the star HD 209458.
作者简介
E. Bekesov
Sternberg Astronomical Institute; Moscow State University
Email: egor03121996@mail.ru
Moscow, Russia; Moscow, Russia
A. Cherepashchuk
Sternberg Astronomical Institute; Moscow State University
编辑信件的主要联系方式.
Email: cherepashchuk@gmail.com
Moscow, Russia; Moscow, Russia
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