The accretion rates-luminosity relations and evolutionary sequence of FSRQs, BL Lac objects and radio galaxies | |
Xie GZ(谢光中)1,2; Zhou SB(周曙白)1,2; Liu HT(刘洪涛)1; Chen LE(陈洛恩)1; Ma L(马力)1; Xie, GZ (reprint author), Chinese Acad Sci, Natl Astron Observ, Yunnan Observ, POB 110, Kunming 650011, Peoples R China. | |
发表期刊 | INTERNATIONAL JOURNAL OF MODERN PHYSICS D |
2004-02 | |
卷号 | 13期号:2页码:347-357 |
DOI | 10.1142/S0218271804004670 |
产权排序 | 第1完成单位 |
收录类别 | SCI |
关键词 | Galaxy Evolution Galactic Nuclei Active Galaxy Quasars Black Hole Physics |
摘要 | A: sample of 39 blazars with well-established rapid variability timescale and bolometric luminosity has been compiled from literature. Based on the assumption that central supermassive black holes (SMBHs) are Kerr black holes, the upper limits of SMBHs were estimated. The masses ranged from 10(7.2)M(circle dot) to 10(9.4)M((C)), showing a distribution of three subclasses: massive flat spectra radio quasars (FSRQs) and smaller mass BL Lacs, occupy separate regions, while medium mass FSRQ and BL Lac object bridge the gap. In addition, we complied a sample of radio galaxies including 9 sources for which their black holes masses have been derived from the M-BH - sigma correlation and their optical and infrared data have been well observed. We find that the intrinsic accretion rates axe quite different between FSRQs, BL Lacs and the radio galaxies. The diagram of the intrinsic accretion rate-luminosity relations shows that FSRQs occur in the earlier, high luminosity, violent phase of galactic evolution sequence, while BL Lacs occur in the low luminosity, transition phase between quasars and radio galaxies, and the radio galaxies occur in the late stage of the elliptical galaxy evolution sequence. Our theoretical results prove that the evolutionary track of the elliptical galaxy evolutionary sequence is from FSRQs to BL Lacs and then to the radio galaxies. The evolution diagram of blazars derived in this paper seems to be similar to Hertzsprung-Russell diagram of star evolution. |
语种 | 英语 |
学科领域 | Astronomy & Astrophysics |
文章类型 | Article |
ISSN | 0218-2718 |
URL | 查看原文 |
归档日期 | 2004-04-21 |
WOS记录号 | WOS:000220610500012 |
WOS研究方向 | Astronomy & Astrophysics |
WOS类目 | Astronomy & Astrophysics |
关键词[WOS] | SUPERMASSIVE BLACK-HOLES ; RAY-LOUD BLAZARS ; SPECTRAL ENERGY-DISTRIBUTIONS ; ACTIVE GALACTIC NUCLEI ; HISTORICAL LIGHT-CURVE ; QUASI-STELLAR OBJECTS ; GAMMA-RAY ; LACERTAE OBJECTS ; PERIODIC ANALYSIS ; HOST GALAXIES |
引用统计 | |
文献类型 | 期刊论文 |
条目标识符 | http://ir.ynao.ac.cn/handle/114a53/6982 |
专题 | 星系研究组 |
通讯作者 | Xie, GZ (reprint author), Chinese Acad Sci, Natl Astron Observ, Yunnan Observ, POB 110, Kunming 650011, Peoples R China. |
作者单位 | 1.National Astronomical Observatories/Yunnan Observatory, Chinese Academy of Sciences, P.O. Box 110, Kunming 650011, P. R. China 2.Yunnan Astrophysics Center, Physics Department, Yunnan University, Kunming 650091, P. R. China |
第一作者单位 | 中国科学院云南天文台 |
推荐引用方式 GB/T 7714 | Xie GZ,Zhou SB,Liu HT,et al. The accretion rates-luminosity relations and evolutionary sequence of FSRQs, BL Lac objects and radio galaxies[J]. INTERNATIONAL JOURNAL OF MODERN PHYSICS D,2004,13(2):347-357. |
APA | Xie GZ,Zhou SB,Liu HT,Chen LE,Ma L,&Xie, GZ .(2004).The accretion rates-luminosity relations and evolutionary sequence of FSRQs, BL Lac objects and radio galaxies.INTERNATIONAL JOURNAL OF MODERN PHYSICS D,13(2),347-357. |
MLA | Xie GZ,et al."The accretion rates-luminosity relations and evolutionary sequence of FSRQs, BL Lac objects and radio galaxies".INTERNATIONAL JOURNAL OF MODERN PHYSICS D 13.2(2004):347-357. |
条目包含的文件 | ||||||
文件名称/大小 | 文献类型 | 版本类型 | 开放类型 | 使用许可 | ||
THE ACCRETION RATES–(188KB) | 期刊论文 | 作者接受稿 | 开放获取 | CC BY-NC-SA | 浏览 请求全文 |
除非特别说明,本系统中所有内容都受版权保护,并保留所有权利。
修改评论