The Origin and evolution of galaxies : proceedings of the NATO Advanced Study Institute held at Erice, Italy, May 11-23, 1981, VIIth course of the International School of Cosmology and Gravitation
著者
書誌事項
The Origin and evolution of galaxies : proceedings of the NATO Advanced Study Institute held at Erice, Italy, May 11-23, 1981, VIIth course of the International School of Cosmology and Gravitation
(NATO advanced study institutes series, ser. C . Mathematical and physical sciences ; v. 97)
D. Reidel , Sold and distributed in the U.S.A. and Canada by Kluwer Boston Inc., c1983
- :pbk
大学図書館所蔵 全22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
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  ノルウェー
  アメリカ
注記
Includes bibliographies and index
内容説明・目次
- 巻冊次
-
ISBN 9789027715074
内容説明
The Origin and Evolution of Galaxies is the outstanding problem of modern cosmology. Fortunately. we have a firm cosmological framework on which to base our theories (the hot big bang) and recently there has been substantial progress in providing observations which potentially can constrain these theories. The problem of galaxy formation is. as a consequence. one involving many diverse branches of physics and astrophysics. It has been the aim of the school. and this compendium of lectures and seminars. to bring together these diverse aspects at a level enabling research workers to understand what is going on in other corners of the subject and to see how progress in each area impinges on the others. We are grateful to the contributors to this volume for allowing us considerable editorial license with their articles. We have attempted to provide a representative sample of the talks that were given at the school besides the texts of the invited lecturers. It is regrettable that for reasons of space we have had to leave out a number of other contributions.
目次
Inaugural lecture.- Relativistic cosmology for astrophysicists.- Numerical cosmologies.- Grand unification and cosmology.- Theory and evidence about the origin of cosmological structure.- Adiabatic vs. isothermal: two pictures of galaxy origin.- Structure in the universe and fluctuations in the cosmic microwave background.- Large-scale fluctuations in the mass distribution and the microwave background: nature and evolution.- Evolution of potential perturbations after decoupling (the adiabatic scenario).- Primordial stars — the precursors to galaxy formation.- Very massive objects and pregalactic stars.- The chemical evolution of galaxies.- Stellar dynamical processes and the evolution of galaxies and galaxy clusters.- Disc stability and halo mass.- Evolution of faint galaxies.- Cosmological evolution of QSOs and radio galaxies.- Clusters of galaxies.- Epilogue: do we understand how galaxies formed?.
- 巻冊次
-
:pbk ISBN 9789027715173
内容説明
The Origin and Evolution of Galaxies is the outstanding problem of modern cosmology. Fortunately. we have a firm cosmological framework on which to base our theories (the hot big bang) and recently there has been substantial progress in providing observations which potentially can constrain these theories. The problem of galaxy formation is. as a consequence. one involving many diverse branches of physics and astrophysics. It has been the aim of the school. and this compendium of lectures and seminars. to bring together these diverse aspects at a level enabling research workers to understand what is going on in other corners of the subject and to see how progress in each area impinges on the others. We are grateful to the contributors to this volume for allowing us considerable editorial license with their articles. We have attempted to provide a representative sample of the talks that were given at the school besides the texts of the invited lecturers. It is regrettable that for reasons of space we have had to leave out a number of other contributions.
目次
Inaugural lecture.- Relativistic cosmology for astrophysicists.- Numerical cosmologies.- Grand unification and cosmology.- Theory and evidence about the origin of cosmological structure.- Adiabatic vs. isothermal: two pictures of galaxy origin.- Structure in the universe and fluctuations in the cosmic microwave background.- Large-scale fluctuations in the mass distribution and the microwave background: nature and evolution.- Evolution of potential perturbations after decoupling (the adiabatic scenario).- Primordial stars - the precursors to galaxy formation.- Very massive objects and pregalactic stars.- The chemical evolution of galaxies.- Stellar dynamical processes and the evolution of galaxies and galaxy clusters.- Disc stability and halo mass.- Evolution of faint galaxies.- Cosmological evolution of QSOs and radio galaxies.- Clusters of galaxies.- Epilogue: do we understand how galaxies formed?.
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