云南师范大学学报（自然科学版）
雲南師範大學學報（自然科學版）
운남사범대학학보（자연과학판）
JOURNAL OF YUNAN NORMAL UNIVERSITY(NATURAL SCIENCES EDITION)
2014年
6期
30-34
,共5页
Blazar天体:黑洞质量%吸积率:热光度
Blazar天體:黑洞質量%吸積率:熱光度
Blazar천체:흑동질량%흡적솔:열광도
Blazar%Black hole mass%Accretion rate%Bolometric luminosity
收集了109个 blazar天体(HBLs 51个,LBLs 40个,FSRQs 18个)的相关观测数据,对该样本的黑洞质量、吸积率、热光度和红移的分布规律进行了统计分析,讨论了吸积率与热光度、黑洞质量与热光度之间的关系,结果发现：(1)存在一个从 FSRQs经 LBLs到 HBLs 的演化序列；(2)爱丁顿吸积率是影响 blazar天体三个子类之间演化序列的主要因素；(3)blazar 天体三个子类的热光度需要进行多普勒效应改正。
收集瞭109箇 blazar天體(HBLs 51箇,LBLs 40箇,FSRQs 18箇)的相關觀測數據,對該樣本的黑洞質量、吸積率、熱光度和紅移的分佈規律進行瞭統計分析,討論瞭吸積率與熱光度、黑洞質量與熱光度之間的關繫,結果髮現：(1)存在一箇從 FSRQs經 LBLs到 HBLs 的縯化序列；(2)愛丁頓吸積率是影響 blazar天體三箇子類之間縯化序列的主要因素；(3)blazar 天體三箇子類的熱光度需要進行多普勒效應改正。
수집료109개 blazar천체(HBLs 51개,LBLs 40개,FSRQs 18개)적상관관측수거,대해양본적흑동질량、흡적솔、열광도화홍이적분포규률진행료통계분석,토론료흡적솔여열광도、흑동질량여열광도지간적관계,결과발현：(1)존재일개종 FSRQs경 LBLs도 HBLs 적연화서렬；(2)애정돈흡적솔시영향 blazar천체삼개자류지간연화서렬적주요인소；(3)blazar 천체삼개자류적열광도수요진행다보륵효응개정。
In this paper,we collected 109 samples of blazar(51 HBLs,40 LBLs,18 FSRQs),then ana-lyzed the statistical distributions of black hole mass,accretion rate,bolometric luminosity and red-shifts of the samples,and discussed the relationship between the black hole mass and the bolo-metric luminosity,and between the accretion rate and the bolometric luminosity.At last,we drew the following conclusions:(1 )There are an evolutionary sequence of properties from FSRQs through LBLs to HBLs;(2)The main reason for the evolutionary sequence of three subclass of blazar may be Edditon ratio rather than black hole mass;(3)The observed bolometric luminosity must be corrected for the Doppler effect.
