Interstellar turbulence
著者
書誌事項
Interstellar turbulence
(Cambridge contemporary astrophysics)
Cambridge University Press, 1999
- hardback
大学図書館所蔵 全6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
注記
Includes bibliographical references
内容説明・目次
内容説明
Turbulence is universal and mysterious. It remains one of the major unsolved problems in physics and astrophysics. From star formation to large-scale outflows, turbulence is present in all interstellar and intergalactic media. With advances in observational techniques (from optical to radio) and the development of more efficient computer codes and faster computers, research in this area has made spectacular progress in recent years. This volume presents a series of review articles covering every aspect of interstellar turbulence - from accretion disks, molecular clouds, atomic and ionized media, through to spiral galaxies - based on a major international conference held in Mexico City. The result is a comprehensive overview of the most important developments in observing and modelling turbulent flows in the cosmos. It provides graduate students and researchers with a state-of-the-art summary of observational, theoretical and computational research in interstellar turbulence.
目次
- 1. Turbulence in the interstellar medium: a retrospective review
- 2. Mechanism of formation of atmospheric turbulence relevant for optical astronomy
- 3. Properties of atomic gas in spiral galaxies
- 4. Turbulence in the ionized gas in spiral galaxies
- 5. Probing interstellar turbulence in the warm ionized medium using emission lines
- 6. The spectrum and galactic distribution of microturbulence in diffuse ionized gas
- 7. Small scale structure and turbulence in the interstellar medium
- 8. What is the Reynolds number of the Reynolds' layer?
- 9. Photoionized gas in the galactic halo
- 10. Turbulent heating of the diffuse ionized gas
- 11. Cosmic rays in interstellar turbulence
- 12. Turbulence in line-driven stellar winds
- 13. An introduction to compressible MHD turbulence
- 14. Turbulence in atomic hydrogen
- 15. Supershells in spiral galaxies
- 16. The size distribution of superbubbles in the interstellar medium
- 17. Large-scale motions in the ISM of elliptical and spiral galaxies
- 18. Vortical motions driven by supernova explosions
- 19. The intermittent dissipation of turbulence: is it observed in the interstellar medium?
- 20. Chemistry in turbulent flows
- 21. Supersonic turbulence in giant extragalactic HII regions
- 22. Turbulence in HII regions: new results
- 23. Hypersonic turbulence of H2O masers
- 24. Water masers tracing alfvenic turbulence and magnetic fields in W51 M and W49 N
- 25. Turbulence in the Ursa Major cirrus cloud
- 26. The collisions of HVCs with a magnetized gaseous disk
- 27. The initial stellar mass function as a statistical sample of turbulent cloud structure
- 28. The structure of molecular clouds: are they fractal?
- 29. Diagnosing properties of turbulent flows from spectral line observations of the molecular interstellar medium
- 30. Centroid velocity increments as a probe of the turbulent velocity field in interstellar molecular clouds
- 31. High-resolution C18O mapping observations of Heiles' cloud 2 - statistical properties of the line width
- 32. Observations of magnetic fields in dense interstellar clouds: implications for MHD turbulence and cloud evolution
- 33. The density PDFs of supersonic random flows
- 34. Turbulence as an organizing agent in the ISM
- 35. Turbulence and magnetic reconnection in the interstellar medium
- 36. The evolution of self-gravitating, magnetized, turbulent clouds: numerical experiments
- 37. Super-Alfvenic turbulent fragmentation in molecular clouds
- 38. Decay timescales of MHD turbulence in molecular clouds
- 39. Numerical magnetohydrodynamic studies of turbulence and star formation
- 40. Direct numerical simulations of compressible magnetohydrodynamical turbulence
- 41. Fragmentation in molecular clouds: the formation of a stellar cluster
- 42. Accretion disk turbulence.
「Nielsen BookData」 より