東京大学
Princeton University
国立天文台 : 総合研究大学院大学(SOKENDAI)
東京大学 : 国立天文台
著者所属（英）
The University of Tokyo
Princeton University
National Astronomical Observatory of Japan : The Graduate University for Advanced Studies (SOKENDAI)
The University of Tokyo : National Astronomical Observatory of Japan
出版者
宇宙航空研究開発機構(JAXA)
出版者（英）
Japan Aerospace Exploration Agency (JAXA)
雑誌名
宇宙航空研究開発機構特別資料
雑誌名(英)
JAXA Special Publication: Proceedings of the SPICA Science Conference from Exoplanets to Distant Galaxies: SPICA's New Window on the Cool Universe
巻
JAXA-SP-17-010E
ページ
353 - 355
発行年
2018-03-09
会議概要（会議名, 開催地, 会期, 主催者等）（英）
SPICA Science Conference from Exoplanets to Distant Galaxies: SPICA's New Window on the Cool Universe (June 18-21, 2013. Ito Hall, the University of Tokyo), Bunkyou-ku, Tokyo, Japan
抄録（英）
Recent simulations and observational data have been used to investigate the possibility of planet-planet scattering or Kozai oscillations to explain the formation of certain non-solar-like planetary systems. Markov Chain Monte Carlo (MCMC) simulations have benefits compared to standard Monte Carlo ones. With these advantages in mind, an advanced three dimensional MCMC simulator has been written to investigate the orbital solutions to the τ Boo system in order to better understand its possible formation history.
内容記述
形態: カラー図版あり
内容記述（英）
Physical characteristics: Original contains color illustrations
Markov Chain Monte Carlo Simulations and Binary Orbital Elements
AA1730027076.pdf
(3.41MB)
