Binaries as tracers of stellar formation
著者
書誌事項
Binaries as tracers of stellar formation
Cambridge Univ. press, 1992
大学図書館所蔵 全8件
  青森
  岩手
  宮城
  秋田
  山形
  福島
  茨城
  栃木
  群馬
  埼玉
  千葉
  東京
  神奈川
  新潟
  富山
  石川
  福井
  山梨
  長野
  岐阜
  静岡
  愛知
  三重
  滋賀
  京都
  大阪
  兵庫
  奈良
  和歌山
  鳥取
  島根
  岡山
  広島
  山口
  徳島
  香川
  愛媛
  高知
  福岡
  佐賀
  長崎
  熊本
  大分
  宮崎
  鹿児島
  沖縄
  韓国
  中国
  タイ
  イギリス
  ドイツ
  スイス
  フランス
  ベルギー
  オランダ
  スウェーデン
  ノルウェー
  アメリカ
内容説明・目次
内容説明
More than two-thirds of stars belong to multiple stellar systems. Binary stars are considered now as one of the best constraints on stellar formation models. Not only do binaries keep memory of their birth conditions but their orbit will also be subjected to changes by tidal effects, wind accretion and encounters in clusters. Certainly the correlation between orbital eccentricity and period is a clue to our understanding of double star history. These proceedings aim to disentangle evidence of stellar formation from later physical evolution. Each article in this 1992 volume is a paper that was read at a meeting organized to honour Dr Roger Griffin of the University of Cambridge for his pioneer work in galactic astronomy, dynamics of clusters and study on binary stars due to his cross-correlation technique to determine stellar radial velocities.
目次
- 1. N-body simulations of primordial binaries and tidal capture in open clusters
- 2. When and how can binary data test similar models?
- 3. Statistical analysis of single-lined red giant spectroscopic binaries
- 4. The formation of binary stars
- 5. Distribution and evolution of orbital elements for 1 M primaries
- 6. Tidal circularization of short period binaries
- 7. Composite-spectrum binaries
- 8. Orbital elements for field late-type binaries
- 9. Evidences for interaction among wide binary systems: to Ba or not to Ba?
- 10. Spectroscopic binaries in the open cluster M67
- 11. Spectroscopic binaries in the halo
- 12. Eccentricity evolution of a binary embedded in a disk
- 13. The eccentricity distribution of pre-main sequence binaries
- 14. A new algorithm to derive the mass-ratio distribution of spectroscopic binaries in open clusters
- 15. Are barium dwarfs progenitors of barium giants
- 16. RZ Eridani as a constraint on synchronization and circularization times
- 17. Ekman layers and tidal synchronization of binary stars
- 18. The distribution of mass ration in late-type main-sequence binary systems
- 19. The dynamical evolution of G-type main sequence binaries
- 20. Present state of the tidal theory
- 21. Infrared companions: clues to binary star formation
- 22. The distribution of cutoff periods with age: an observational constraint on tidal circularization theory.
「Nielsen BookData」 より