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Photometry of three gamma-ray-loud quasars and implications for supermassive black holes
Xie GZ(谢光中)1,2,3; Liang EW(梁恩维)1,2,4; Zhou SB(周曙白)1,2,3; Li KH(李开华)1,2; Dai BZ(戴本忠)1,2,3; Ma L(马力)1,2,5; Xie, GZ (reprint author), Chinese Acad Sci, Natl Astron Observ, Yunnan Observ, POB 110, Kunming 650011, Peoples R China.
发表期刊MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
2002-08
卷号334期号:2页码:459-470
DOI10.1046/j.1365-8711.2002.05528.x
产权排序第1完成单位
收录类别SCI
关键词Black Hole Physics Galaxies : Active Galaxies : Nuclei Galaxies : Photometry Quasars : General
摘要The results of photometry of three gamma-ray-loud quasars, PKS 1510-089, 3C 279 and OJ248, during 2001 in the B, V and R bands and implications for the supermassive black hole (SMBH) model in these objects are presented. The results show that the three quasars had significant, but irregular, rapid outbursts with a typical time-scale of about 40-60 min and a typical amplitude of about Deltam similar or equal to0.60-1.26 mag during the observations. For 3C 279 and OJ248 the upper limits of the masses of SMBHs are estimated from the observed minimum optical variability time-scale, and the lower limits are also estimated by a method proposed by Dermer & Gehrels. The masses derived from both methods are reasonable. For PKS 1510-089 a new brightness minima was also observed. Analysing the observations from 1999 to 2001, three minima were observed. Although their light curves are poorly sampled, it is intriguing to note that these minimum at intervals of about 43 min seem to indicate the possibility of a periodic phenomenon. So a hypothesis is proposed to interpret the phenomenon, suggesting that there is a binary black hole system at the centre. The parameters of the system are estimated by a very simple method. The periodicity is about 336+/-14 d in the observed frame; the masses of the primary and secondary black holes are 10(8.0) and 10(6.2) M-circle dot, respectively; the distance between two black holes is 10(15.81) cm (378R (g) of the primary black hole), and the lifetime of the system is 10(6.0) yr. These results seem to indicate that PKS 1510-089 is another possible candidate binary black hole system. It should be monitored in future to obtain more data for further analysis to test the hypothesis.
语种英语
学科领域Astronomy & Astrophysics
文章类型Article
ISSN0035-8711
URL查看原文
归档日期2002-10-14
WOS记录号WOS:000177258500024
WOS研究方向Astronomy & Astrophysics
WOS类目Astronomy & Astrophysics
关键词[WOS]ACTIVE GALACTIC NUCLEI ; BL-LACERTAE OBJECTS ; RADIO-SOURCES ; BLAZARS ; VARIABILITY ; RADIATION ; OJ-287 ; JET ; MARKARIAN-421 ; PRECESSION
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被引频次:55[WOS]   [WOS记录]     [WOS相关记录]
文献类型期刊论文
条目标识符http://ir.ynao.ac.cn/handle/114a53/6949
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.Yunnan Observatory, National Astronomical Observatories, Chinese Academy of Sciences, PO Box 110, Kunming 650011, China
2.United Laboratory of Optical Astronomy, Chinese Academy of Sciences
3.Yunnan Astrophysics Center, Yunnan University, Kunming 650091, China
4.Physics Department, Guangxi University, Nanning, Guangxi 530004, China
5.Physics Department, Yunnan Normal University, Kunming 650092, China
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Xie GZ,Liang EW,Zhou SB,et al. Photometry of three gamma-ray-loud quasars and implications for supermassive black holes[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2002,334(2):459-470.
APA Xie GZ.,Liang EW.,Zhou SB.,Li KH.,Dai BZ.,...&Xie, GZ .(2002).Photometry of three gamma-ray-loud quasars and implications for supermassive black holes.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,334(2),459-470.
MLA Xie GZ,et al."Photometry of three gamma-ray-loud quasars and implications for supermassive black holes".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 334.2(2002):459-470.
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