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  • 标题:A realistic two-dimensional model of Altair ⋆
  • 本地全文:下载
  • 作者:K. Bouchaud ; A. Domiciano de Souza ; M. Rieutord
  • 期刊名称:Astronomy & Astrophysics
  • 印刷版ISSN:0004-6361
  • 电子版ISSN:1432-0746
  • 出版年度:2020
  • 卷号:633
  • 页码:1-20
  • DOI:10.1051/0004-6361/201936830
  • 语种:English
  • 出版社:EDP Sciences
  • 摘要:Context.Fast rotation is responsible for important changes in the structure and evolution of stars and the way we see them. Optical long baseline interferometry now allows for the study of its effects on the stellar surface, mainly gravity darkening and flattening.Aims.We aim to determine the fundamental parameters of the fast-rotating star Altair, in particular its evolutionary stage (represented here by the core hydrogen mass fractionXc), mass, and differential rotation, using state-of-the-art stellar interior and atmosphere models together with interferometric (ESO-VLTI), spectroscopic, and asteroseismic observations.Methods.We use ESTER two-dimensional stellar models to produce the relevant surface parameters needed to create intensity maps from atmosphere models. Interferometric and spectroscopic observables are computed from these intensity maps and several stellar parameters are then adjusted using the publicly available MCMC algorithm Emcee.Results.We determined Altair’s equatorial radius to beReq = 2.008 ± 0.006 R⊙, the position angle PA = 301.1 ± 0.3°, the inclinationi = 50.7 ± 1.2°, and the equatorial angular velocity Ω = 0.74 ± 0.01 times the Keplerian angular velocity at equator. This angular velocity leads to a flattening ofε = 0.220 ± 0.003. We also deduce from the spectroscopically derivedvsini ≃ 243 km s−1, a true equatorial velocity of ∼314 km s−1corresponding to a rotation period of 7h46m (∼3 cycles/day). The data also impose a strong correlation between mass, metallicity, hydrogen abundance, and core evolution. Thanks to asteroseismic data, and provided our frequencies identification is correct, we constrain the mass of Altair to 1.86 ± 0.03M⊙and further deduce its metallicityZ = 0.019 and its core hydrogen mass fractionXc = 0.71, assuming an initial solar hydrogen mass fractionX = 0.739. These values suggest that Altair is a young star ∼100 Myr old. Finally, the 2D ESTER model also gives the internal differential rotation of Altair, showing that its core rotates approximately 50% faster than the envelope, while the surface differential rotation does not exceed 6%.
  • 关键词:enstars: individual: Altairstars: interiorsstars: atmospheresstars: rotationstars: fundamental parametersstars: oscillations
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