Populations of high energy sources in galaxies : proceedings of the 230th symposium of the international astronomical union held in Dublin, Ireland 15-19 August 2005
著者
書誌事項
Populations of high energy sources in galaxies : proceedings of the 230th symposium of the international astronomical union held in Dublin, Ireland 15-19 August 2005
(IAU symposium and colloquium proceedings series, . IAU Symposium ; no. 230)
Cambridge University Press, c2006
大学図書館所蔵 全11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
At head of title: International Astronomical Union, Union Astronomique Internationale
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内容説明・目次
内容説明
For the last 40 years astronomers have observed sources of intense X-ray radiation from beyond our Solar System. These have been associated with remarkable objects, such as neutron stars and black holes. Current satellite observatories have enabled us to extend the studies of these objects from the Milky Way and Magellanic Clouds to individual X-ray sources in other galaxies. At the same time, imaging facilities at gamma-rays and TeV energies have improved enormously, leading to many further discoveries within our own galaxy. This Symposium presents an overview of these new developments, covering detailed studies of individual sources within the Milky Way, global descriptions of X-ray source populations in other galaxies, and less resolved relatives at high redshift. Galaxy nuclei and diffuse emission components are included, as are new discoveries at gamma-rays and TeV energies. IAU S230 is a valuable resource for astronomers and graduates working in high-energy astrophysics.
目次
- Preface
- Introduction
- 1. Key source categories on our galaxy
- 2. High energy processes in the ISM
- 3. Detailed population studies in the nearer galaxies
- 4. Source classes that emerge from sampling over galaxies
- 5. Overall population characteristics
- 6. High energy population synthesis
- 7. The high-redshift context
- Closing remarks.
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