Decrease of Velocity Differences between Baryonic Objects and Cold Dark Matter : Progress Letters
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概要
- 論文の詳細を見る
It is investigated whether observed large-scale streaming of galaxies represents velocities of dark matter under explosion scenarios. It seems that, although individual galaxies will not represent motions of dark matter, cluster of galaxies follows the velocity field of dark matter. The origin and upper limits of such field are considered.
- 理論物理学刊行会の論文
- 1990-04-25
著者
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HARA Tetsuya
Department of Anesthesiology, Nagasaki University School of Medicine
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Hariu T.
Yamagata University
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MIYOSHI Shigeru
Department of Physics, Kyoto Sangyo University
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Hara Tetsuya
Research Institute For Fundamental Physics Kyoto University
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Miyoshi Shigeru
Department Of Physics Kyoto Sangyo University
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HARA Takashi
Institute of Physics, College of Arts and Sciences University of Tokyo
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Hara Tetsuya
Department Of Anesthesiology Nagasaki Rosai Hospital
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HARA Takashi
Institute of Physics, College of Arts and Science University of Tokyo : Courant Institute of Mathematical Sciences, New York University
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HARA Tetsuya
Department of Physics, Kyoto University
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Miyoshi Sigeru
Department of Physics, Kyoto Sangyo University
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Hara Tetsuya
Research Center for Nuclear Physics, Osaka. University
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