Evolution from Distant Star-Forming Galaxies to Nearby Elliptical Galaxies 遠方の星生成銀河から近傍の楕円銀河への進化
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Bibliographic Information
- Title
-
Evolution from Distant Star-Forming Galaxies to Nearby Elliptical Galaxies
- Other Title
-
遠方の星生成銀河から近傍の楕円銀河への進化
- Author
-
高木, 俊暢
- Author(Another name)
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タカギ, トシノブ
- University
-
立教大学
- Types of degree
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博士 (理学)
- Grant ID
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甲第109号
- Degree year
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2001-03-31
Note and Description
博士論文
資料形態 : テキストデータ プレーンテキスト
コレクション : 国立国会図書館デジタルコレクション > デジタル化資料 > 博士論文
学位論文本体及び論文要旨 : 1-72コマ
参考論文は、国立国会図書館内でのみ閲覧できます。
Table of Contents
- Abstract
- Contents
- 1 Introduction
- 2 SED Model of Star-Forming Galaxies
- 2.1 Introduction
- 2.2 Stellar SED Model
- 2.3 Dust Model
- 2.4 Radiative Transfer
- 2.5 Sensitivity Analyses
- 2.6 Evolutionary Model
- 2.7 Evolutionary Behaviors of Model
- 2.8 Summary
- 3 Starburst Galaxies in the Local Universe
- 3.1 Introduction
- 3.2 Arp220 and M82
- 3.3 UV-Selected Starburst Galaxies
- 3.4 Ultraluminous Infrared Galaxies
- 3.5 Discussion
- 3.6 Conclusions
- 4 Major Star Formation in Elliptical Galaxies
- 4.1 Introduction
- 4.2 Candidates of Star-Forming Ellipticals
- 4.3 Evolutionary Path from Star-Forming Galaxies to Ellipticals
- 4.4 Formation of Ellipticals in the Cosmic Star Formation History
- 4.5 Discussion
- 4.6 Conclusions
- 5 Gone with Galactic Winds:Outflowing Dust from Star-Forming Ellipticals
- 5.1 Introduction
- 5.2 Intracluster Dust Emission
- 5.3 A Nearby Cluster:Coma
- 5.4 FIR Emission from Clusters at High Redshifts
- 5.5 Discussion
- 5.6 Conclusions
- 6 Concluding Remarks
- AGE AND DUST DEGENERACY FOR STARBURST GALAXIES SOLVED?
