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赛弗特工星系黑洞质量与宇宙学红移的研究
引用本文:黄霞,张雄,熊定荣. 赛弗特工星系黑洞质量与宇宙学红移的研究[J]. 云南师范大学学报(自然科学版), 2013, 0(6): 41-44
作者姓名:黄霞  张雄  熊定荣
作者单位:云南师范大学物理与电子信息学院,云南昆明650500
基金项目:国家自然科学基金资助项目(11163007,U1231203);云南省引力理论创新团队资助项目;云南省高校天体物理创新团队资助项目.
摘    要:
对214个SeyfertI星系(其中147个窄线SeyfertI星系(NLSIs),67个宽线Seyfert工星系(BLSIs))的红移、热光度、爱丁顿比、黑洞质量的分布进行研究,并讨论了红移和热光度、爱丁顿比的关系。得到了以下结论:1)窄线SeyfertI星系的红移、热光度、爱丁顿比都大于宽线SeyfertI星系的红移、热光度、爱丁顿比;2)窄线SeyfertI星系的黑洞质量小于宽线SeyfertI星系的黑洞质量;3)在大样本下SeyfertI星系从窄线Seyfert工星系到宽线SeyfertI星系演化,与他人用其他方法得到的结果是一致的。

关 键 词:Seyfert  I星系  红移  热光度  爱丁顿比  黑洞质量

The Research about Black Hole Mass and Cosmological Redshift in Seyfert I
Affiliation:HUANG Xia, ZHANG Xiong, XlONG Ding-rong (School of Physics and Electronic Information,Yunnan Normal University,Kunming 650500,China)
Abstract:
The distribution of the bolometric luminosity, redshift, Eddington ratio and the black hole mass of 214 Seyfert I galaxies(including 147 narrow line Seyfert I galaxies and 67 broad line Seyfert I galaxies)were studied and the relationships between bolometric luminosity and redshift, between red- shift and Eddington ratio were discussed. The results showed that: 1) The bolometric luminosity, redshi{t, Eddington ratio of the narrow line Seyfert I galaxies is greater than that of the broad line Seyfert I galaxies; 2) Black hole mass of the narrow line Seyfert I galaxies is less than that of the broad line Seyfert I galaxies; 3) On large numbers of samples, the evolutionary process of Seyfert galaxies is from the narrow line Seyfert I to the broad line Seyfert I, which is the same as others.
Keywords:Seyfert 1 galaxies  Redshift  Bolometric luminosity  Eddington ratio  Black hole mass
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