Optical multi-color monitoring of OJ 287 from 2006 to 2012

被引:0
作者
Qian Guo [1 ,2 ,3 ,4 ]
Ding-Rong Xiong [1 ,2 ,3 ]
Jin-Ming Bai [1 ,2 ,3 ]
Xu-Liang Fan [1 ,2 ,3 ,4 ]
Wei-Min Yi [1 ,2 ,3 ]
机构
[1] Yunnan Observatories, Chinese Academy of Sciences
[2] Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences
[3] Center for Astronomical Mega-Science, Chinese Academy of Sciences
[4] University of Chinese Academy of Sciences
关键词
BL Lacertae objects; individual(OJ 287)—galaxies; active—galaxies; photometry;
D O I
暂无
中图分类号
P157.7 [射电星系、特殊星系];
学科分类号
070401 ;
摘要
We present our optical multi-color monitoring of the BL Lac object OJ 287 from January 2006to December 2012 in the V,R and I bands.A relatively active state in OJ 287 has been found over all monitored epochs,among which the variations of average magnitude in V/R/I bands were measured with ?V=1.956 mag,?R=2.067 mag and ?I=2.115 mag,respectively.No reliable intraday variability is detected,but possible variability is detected on 16 nights.Their relative variation amplitudes fall into the range between 1% and 8%,with the majority between 2% and 4%.No time lags have been detected,but strong correlations exist among light curves in the three wavebands.The bluer-when-brighter trend is dominant over intraday timescales,which supports the shock-in-jet model.When combining with additional V/R band data obtained from SMARTS and the Steward Observatory,we also find a bluer-when-brighter trend over a long-term timescale.Some possible periods of 513,176,36,30,26,17 and 14 d are found in all time-series data sets from 2006 to 2017.Possible explanations about these periods are given.
引用
收藏
页码:59 / 70
页数:12
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