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CALIBRATION OF STELLAR PARAMETERS OF 85 PEG SYSTEM
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  • CALIBRATION OF STELLAR PARAMETERS OF 85 PEG SYSTEM
  • CALIBRATION OF STELLAR PARAMETERS OF 85 PEG SYSTEM
저자명
Bach. Kiehunn,Kim. Yong-Cheol,Demarque. Pierre
간행물명
韓國宇宙科學會誌
권/호정보
2007년|24권 1호|pp.31-38 (8 pages)
발행정보
한국우주과학회
파일정보
정기간행물|ENG|
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이 논문은 한국과학기술정보연구원과 논문 연계를 통해 무료로 제공되는 원문입니다.
서지반출

기타언어초록

We have investigated the evolutionary status of 85 Peg within the framework of standard evolutionary theory. 85 Peg has been known to be a visual and spectroscopic binary system in the solar neighborhood. In spite of the accurate information of the total mass (${sim}1.5M_{odot}$) and the distance (${sim}12pc$) from the HIPPARCOS parallax, it has been undetermined an individual mass, therefore the evolved status of the system. Moreover, the coupled uncertainties of chemical composition and age, make matters worse in predicting an evolutionary status of the system. Nevertheless, we computed the various possible models for 85 Peg, and then calibrated stellar parameters by adjusting to the recent observational data. Our modelling computation has included recently updated input physics and stellar theory such as opacity, equation of state, and chemical diffusion. Through a statistical assessment, we have derived a confident parameter set as the best solution which minimized $X^{2}$ within the observational error domain. Most of all, we found that 85 Peg is not a binary system but a triple system with an unseen companion 85 Peg $B_{b};{sim}0.16M_{odot}$. The aim of the present paper is (1) to provide a complete modelling of the stellar system based on the evolutionary theory, and (2) to constrain the physical dimensions such as mass, metallicity and age.