The Mount Wilson Observatory : breaking the code of cosmic evolution
著者
書誌事項
The Mount Wilson Observatory : breaking the code of cosmic evolution
(Centennial history of the Carnegie Institution of Washington, v. 1)
Cambridge University Press, 2012
- : pbk
大学図書館所蔵 全1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
"First published 2004. First paperback edition 2012"--T.p. verso
Includes bibliographical references (p. 598-620) and index
内容説明・目次
内容説明
Since its foundation in 1904, the Mount Wilson Observatory has been at the centre of the development of astrophysics. Perched atop a mountain wilderness, two mammoth solar tower telescopes and the 60- and 100-inch behemoth night-time reflectors were all the largest in the world. Research has centred around two main themes - the evolution of stars and the development of the universe. This first volume in a series of five histories of the Carnegie Institution describes the people and events, the challenges and successes that the Observatory has witnessed. It includes biographical sketches of forty of the most famous Mount Wilson pioneer astronomers working during the first half of the twentieth century. Contemporary photographs illustrate the development and use of some of the innovative instruments that filled the observatory during this time. This story brings together the elements that formed modern theories of stellar evolution and cosmology.
目次
- Foreword Richard A. Meserve
- Acknowledgements
- Prologue
- Part I. Before the Beginning (1542-1904): 1. A telegram
- 2. The origin of a name
- 3. Three observatories for Mount Wilson before the real one
- 4. The creation of the Carnegie Institution and its initial Astronomy Advisory Committee
- Part II. Creation of the Observatory and the First Scientific Results: 5. The instruments of detection: solar telescopes, coelostats, spectrographs and spectra
- 6. Snow, hale, frost and gale: just the right people to study storms on the sun
- 7. Tower telescopes and magnetic fields and cycles
- 8. Pioneers of peering: the scientific staff in the early years (1904-9)
- 9. Solar physics: the intermediate years (1910-30)
- 10. Yet more solar physics: motions on the surface, clocks in the gravity field and the reality of prominences
- Part III. The Beginning of Nighttime Sidereal Astronomy at Mount Wilson: 11. The coming of the 60-inch and 100-inch reflectors
- 12. Life on the mountain
- 13. Anatomy of an observatory
- Part IV. Preparation for an Understanding of Stellar Evolution and Galactic Structure: 14. Galactic structure in the raw
- 15. Spectral classification and the invention of spectroscopic parallaxes
- 16. Radial velocity
- 17. Globular star clusters and the galactocentric revolution
- 18. Galactic rotation: Stromberg, Lindblad and Oort
- 19. The Carnegie Meridian Astrometry Department at the Dudley Observatory
- 20. Absolute magnitudes from direct parallaxes and stellar motions
- 21. Threads leading to the population concept that became the fabric of evolution
- Part V. Physics of the Stars and the Interstellar Medium: 22. Five problems in astrophysics
- 23. Long-term research associates and short-term visitors
- 24. Interstellar gas, instruments and the spiral arms of the galaxy
- Part VI. Observational Cosmology and the Code of Stellar Evolution: 25. Observational cosmology I: galaxy classification and the discovery of cepheids
- 26. Observational cosmology II: the expansion of the universe and the search for the curvature of space
- 27. Down more corridors of time
- 28. The observational approach to stellar evolution
- Epilogue
- Abbreviations
- Notes
- Bibliography
- Index.
「Nielsen BookData」 より