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Time lags between the 22 and 37 GHz bursts of 48 radio-loud AGNs
Deng WG(邓文国)1,2; Bai JM(白金明)1; Zhang, L2; Yang, Xian1,2; Deng, WG (reprint author), Chinese Acad Sci, Natl Astron Observ, Yunnan Observ, Kunming 650011, Peoples R China.
发表期刊CHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS
2008-04
卷号8期号:2页码:195-203
DOI10.1088/1009-9271/8/2/06
产权排序第1完成单位
收录类别SCI
关键词Galaxies : Active Methods : Data Analysis Galaxies : Individual (3c 273 3c 279 3c 345 3c 454.3)
摘要Based on the light curves at 22 and 37 GHz from the Metsahovi monitoring program, we investigate the time lags between the two radio bands for 48 radio-loud AGNs. DCF and ZDCF analyses are applied to the data. Our results show that there is a strong correlation between the two radio frequencies for all the sources, with the variations in the light curves at 37 GHz leading the ones at 22 GHz in general. There is no obvious differences between different sub-class AGNs as regards the time lag. In two sources, it was found that the bursts at the lower frequency lead the ones at the higher frequency. One possible explanation is that electron acceleration dominates the light curve until the radiation reaches the maximum. Some sources, such as 3C 273, 3C 279, 3C 345 and 3C 454.3, have good enough data, so we can calculate their lags burst-by-burst. Our calculations show that different outbursts have different lags. Some bursts have positive lags, most of bursts have no clear lags, and a few have negative lags. This result means that different bursts are triggered by different mechanisms, and the interpretation for the result involves both an intrinsic and a geometric mechanism. The positive lags are well consistent with the shock model, and we use these lags to calculate the typical magnetic field strength of the radiating region.
语种英语
学科领域Astronomy & Astrophysics
文章类型Article
ISSN1009-9271
URL查看原文
归档日期2008-10-07
WOS记录号WOS:000255262600006
WOS研究方向Astronomy & Astrophysics
WOS类目Astronomy & Astrophysics
关键词[WOS]GAMMA-RAY BURSTS ; ACTIVE GALACTIC NUCLEI ; BL-LACERTAE OBJECTS ; EXTRAGALACTIC SOURCES ; OPTICAL VARIATIONS ; CORRELATED RADIO ; SPECTRAL LAGS ; RAPID VARIABILITY ; SHOCK-MODELS ; 87 GHZ
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被引频次:1[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/114a53/7041
专题星系研究组
通讯作者Deng, WG (reprint author), Chinese Acad Sci, Natl Astron Observ, Yunnan Observ, Kunming 650011, Peoples R China.
作者单位1.National Astronomical Observatories/Yunnan Observatory, Chinese Academy of Sciences, Kunming 650011
2.Physics Department, Yunnan University, Kunming 650091
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Deng WG,Bai JM,Zhang, L,et al. Time lags between the 22 and 37 GHz bursts of 48 radio-loud AGNs[J]. CHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS,2008,8(2):195-203.
APA Deng WG,Bai JM,Zhang, L,Yang, Xian,&Deng, WG .(2008).Time lags between the 22 and 37 GHz bursts of 48 radio-loud AGNs.CHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS,8(2),195-203.
MLA Deng WG,et al."Time lags between the 22 and 37 GHz bursts of 48 radio-loud AGNs".CHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS 8.2(2008):195-203.
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