首页    期刊浏览 2024年11月07日 星期四
登录注册

文章基本信息

  • 标题:Visual Orbits of Spectroscopic Binaries with the CHARA Array. III. HD 8374 and HD 24546
  • 本地全文:下载
  • 作者:Kathryn V.Lester ; Francis C.Fekel ; Matthew Muterspaugh
  • 期刊名称:The Astronomical journal
  • 印刷版ISSN:0004-6256
  • 电子版ISSN:1538-3881
  • 出版年度:2020
  • 卷号:160
  • 期号:2
  • 页码:1-14
  • DOI:10.3847/1538-3881/ab8f95
  • 语种:English
  • 出版社:American Institute of Physics
  • 摘要:We present the visual orbits of two long-period spectroscopic binary stars, HD 8374 and HD 24546, using interferometric observations acquired with the CHARA Array and the Palomar Testbed Interferometer. We also obtained new radial velocities from echelle spectra using the APO 3.5 m and Fairborn 2.0 m telescopes. By combining the visual and spectroscopic observations, we solve for the full, three-dimensional orbits and determine the stellar masses and distances to within 3% uncertainty. We then estimate the effective temperature and radius of each component star through Doppler tomography and spectral energy distribution analyses, in order to compare the observed stellar parameters to the predictions of stellar evolution models. For HD 8374, we find masses of M1 = 1.636 ± 0.050Me and M2 = 1.587 ± 0.049Me, radii of R1 = 1.84 ± 0.05Re and R2 = 1.66 ± 0.12Re, temperatures of Teff 1 =  7280 110 K and Teff 2 =  7280 120 K, and an estimated age of 1.0 Gyr. For HD 24546, we find masses of M1 = 1.434 ± 0.014Me and M2 = 1.409 ± 0.014Me, radii of R1 = 1.67 ± 0.06Re and R2 = 1.60 ± 0.10Re, temperatures of Teff 1 =  6790 120 K and Teff 2 =  6770 90 K, and an estimated age of 1.4 Gyr. HD 24546 is therefore too old to be a member of the Hyades cluster, despite its physical proximity to the group.
国家哲学社会科学文献中心版权所有