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REDSHIFT DISTRIBUTION AND EVOLUTION FUNCTION OF QUASI-STELLAR OBJECTS

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【作者】 周又元胡岳东

【Author】 ZHOU YOU-YUAN;HU YUE--DONG;China Center of Advanced Science and Technology (World Laboratory), Beijing 100080, PRC Center for Astrophysics, University of Science and Technology of China. Hefei 230026. PRC Center for Astrophysics, University of Science and Technology of China, Hefei 230026, PRC

【机构】 China Center of Advanced Science and Technology (World Laboratory)Beijing 100080PRC Center for AstrophysicsUniversity of Science and Technology of China. Hefei 230026. PRCCenter for AstrophysicsUniversity of Science and Technology of ChinaHefei 230026PRC

【摘要】 <正> Taking account of the selection effect in the line identification, under the cosmologicalredshift hypothesis we calculate the redshift-distribution functions of quasi-stellar objects(QSOs) selected with the slitless technique, using three kinds of evolution functions forQSOs, i. e. the Schmidt-Green function, the Mathez function and the Heisler-Ostriker func-tion, and compare them with the observed distribution. The comparison shows that withregards to both the global behavior and the detailed properties, the predictions agree wellwith observations. We also tried to throw light on the redshift distribution of radio-selectedand color-selected QSOs. Therefore, the obtained results draw to the conclusion that thecosmological-redshift hypothesis is compatible with the redshift distibution of QSOs. Using the redshift distribution of QSOs, we also compare various evolution functionswith observations, and indicate which functions in what range can well explain the observeddistributions.

【Abstract】 Taking account of the selection effect in the line identification, under the cosmologicalredshift hypothesis we calculate the redshift-distribution functions of quasi-stellar objects(QSOs) selected with the slitless technique, using three kinds of evolution functions forQSOs, i. e. the Schmidt-Green function, the Mathez function and the Heisler-Ostriker func-tion, and compare them with the observed distribution. The comparison shows that withregards to both the global behavior and the detailed properties, the predictions agree wellwith observations. We also tried to throw light on the redshift distribution of radio-selectedand color-selected QSOs. Therefore, the obtained results draw to the conclusion that thecosmological-redshift hypothesis is compatible with the redshift distibution of QSOs. Using the redshift distribution of QSOs, we also compare various evolution functionswith observations, and indicate which functions in what range can well explain the observeddistributions.

【基金】 Project partially supported by the National Natural Science Foundation of China.
  • 【文献出处】 Science in China,Ser.A ,中国科学A辑(英文版) , 编辑部邮箱 ,1991年05期
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