Rapid optical variability of gamma-raye-loud blazars | |
Dai BZ(戴本忠)1,2,3,4; Xie GZ(谢光中)1,2,3,4; Li KH(李开华)1,2; Zhou SB(周曙白)1,2,3,4; Liu WW(刘威卫)1,2; Jiang ZJ(姜泽军)1,4; Xie, GZ (reprint author), Chinese Acad Sci, Yunnan Astron Observ, POB 110, Kunming 650011, Peoples R China. | |
发表期刊 | ASTRONOMICAL JOURNAL |
2001-12 | |
卷号 | 122期号:6页码:2901-2912 |
DOI | 10.1086/324450 |
产权排序 | 第1完成单位 |
收录类别 | SCI |
关键词 | Bl Lacertae Objects : General Galaxies : Active Galaxies : Photometry Quasars : General |
摘要 | We present the optical (B, V, and R) photometry for nine GeV and/or TeV gamma -ray blazars, which were observed from 2000 through 2001 with the 1 m telescope at Yunnan Astronomical Observatory. The GeV gamma -ray-loud source PKS 1510-089 was very active during our observation period, showing an apparent variation of 2.0 mag within 41 minutes in the R band. This is the most violently rapid variability in our optical monitoring program since 1982. Some physics parameters are calculated for this source, namely, the emission size, Doppler factor delta, the efficiency (eta) for conversion of accreted matter into energy, and luminosity. An eta = 62.2 was obtained, strongly implying that relativistic beaming is responsible for the rapid variability of the gamma -ray-loud source. The influence of variable seeing conditions on the observations was investigated. There is a weak correlation between the observed variability and the local seeing conditions for the object 1ES 2344+51.4. |
语种 | 英语 |
学科领域 | Astronomy & Astrophysics |
文章类型 | Article |
ISSN | 0004-6256 |
URL | 查看原文 |
归档日期 | 2002-02-27 |
WOS记录号 | WOS:000172932200008 |
WOS研究方向 | Astronomy & Astrophysics |
WOS类目 | Astronomy & Astrophysics |
关键词[WOS] | BL-LACERTAE OBJECTS ; ACTIVE GALAXY MARKARIAN-421 ; HIGH-ENERGY FLARE ; INTRADAY VARIABILITY ; X-RAY ; COMPARISON STARS ; PHOTOMETRIC SEQUENCES ; EXTRAGALACTIC SOURCES ; GALACTIC NUCLEI ; VRI PHOTOMETRY |
引用统计 | |
文献类型 | 期刊论文 |
条目标识符 | http://ir.ynao.ac.cn/handle/114a53/6931 |
专题 | 星系研究组 |
通讯作者 | Xie, GZ (reprint author), Chinese Acad Sci, Yunnan Astron Observ, POB 110, Kunming 650011, Peoples R China. |
作者单位 | 1.Yunnan Astronomical Observatory, Chinese Academy of Sciences, P.O. Box 110, Kunming 650011, China 2.National Astronomical Observatories, Chinese Academy of Sciences, Beijing, China 3.United Laboratory of Optical Astronomy, Chinese Academy of Sciences, Beijing, China 4.Yunnan Astrophysics Center, Yunnan University, Kunming 650091, 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 | Dai BZ,Xie GZ,Li KH,et al. Rapid optical variability of gamma-raye-loud blazars[J]. ASTRONOMICAL JOURNAL,2001,122(6):2901-2912. |
APA | Dai BZ.,Xie GZ.,Li KH.,Zhou SB.,Liu WW.,...&Xie, GZ .(2001).Rapid optical variability of gamma-raye-loud blazars.ASTRONOMICAL JOURNAL,122(6),2901-2912. |
MLA | Dai BZ,et al."Rapid optical variability of gamma-raye-loud blazars".ASTRONOMICAL JOURNAL 122.6(2001):2901-2912. |
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