Gas Flows and Gas Contents in Globular Clusters
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概要
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The flow of gas injected from stars in globular clusters is numerically studied by means of the time-dependent beam scheme. By using structural parameters derived by Peterson and King (1975) and taking radiative cooling and ultraviolet heating into account, we obtain the time variation of velocity, temperature and density distributions in the gas flows in nine globular clusters. Flow in NGC 7078 for the specific mass loss rate of 5.34×10^<-20> sec^<-1> is inward within a stagnation point and is outward outside it after a steady state is realized. As the mass loss rate increases, the velocity of the inward flow increases because of the increase in effective cooling. In the clusters with large gravitational fields, gas becomes partial flow as well as in NGC 7078. However, gas flows wholly outwardly in the clusters with weak fields, and heating causes the increase of the velocity of outflow. From the comparison of the cooling time with flow time, it is suggested that the partial inflow is expected in clusters with the gravitational potential of the cluster core greater than 1.0×10^<12> erg g^<-1>. The gas content in the clusters is also compared with observed data.
- 理論物理学刊行会の論文
- 1979-08-25
著者
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TANAKA Yasutoshi
Department of Physics, Florida State University
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Hirayama Yuzo
Department Of Physics Hokkaido University
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FUKUDA Takashi
Research Institute for Theoretical Physics Hiroshima University
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TANAKA Yasuo
Faculty of Education, Ibaraki University
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ISHIZUKA Toshihisa
Department of Physics, Ibaraki University
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FUKUDA Teruko
Faculty of Education, Ibaraki University
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NAKANIWA Junko
Faculty of Education, Ibaraki University
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SUNAOSHI Misako
Faculty of Education, Ibaraki University
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Fukuda Teruko
Faculty Of Education Ibaraki University
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Nakaniwa Junko
Faculty Of Education Ibaraki University
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Sunaoshi Misako
Faculty Of Education Ibaraki University
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Ishizuka Toshihisa
Department Of Physics Hokkaido University
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Tanaka Yasuo
Faculty Of Education Ibaraki University
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FUKUDA Tomokazu
Laboratory of Physics, Osaka Electro-Communication University
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TANAKA Yosuke
Department of Physics, Kyushu Kyouritsu University
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FUKUDA Takashi
Research Institute for Theoretical Physics, Hiroshima University
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FUKUDA Takashi
Research Institute for Theoretical Physics, Hisoshima University
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Hirayama Yuzo
Department of Physics, Hokkaido University
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