Optical monitoring of 3C 390.3 from 1995 to 2004 and possible periodicities in the historical light curve
Tao, Jun1,2,3; Fan, Junhui4,5; Qian, Bochen1,2,3; Liu, Yi4
刊名ASTRONOMICAL JOURNAL
2008-02-01
卷号135期号:2页码:737-746
关键词galaxies : active galaxies : individual (3C 390.3) galaxies : photometry galaxies : Seyfert methods : data analysis
英文摘要We report V, R, and I band CCD photometry of the radio galaxy 3C 390.3 obtained with the 1.56 m telescope of the Shanghai Astronomical Observatory from 1995 March to 2004 August. Combining these data with data from the literature, we have constructed a historical light curve from 1894 to 2004 and searched for periodicities using the CLEANest program. We find possible periods of 8.30 +/- 1.17, 5.37 +/- 0.49, 3.51 +/- 0.21, and 2.13 +/- 0.08 yr.
学科主题星系与宇宙学研究中心
WOS标题词Science & Technology ; Physical Sciences
类目[WOS]Astronomy & Astrophysics
研究领域[WOS]Astronomy & Astrophysics
关键词[WOS]BALMER EMISSION-LINES ; BL LACERTAE OBJECTS ; X-RAY VARIABILITY ; RADIO GALAXY ; INFRARED VARIABILITY ; SEYFERT-GALAXIES ; N GALAXIES ; 3C-390.3 ; CONTINUUM ; BEHAVIOR
收录类别SCI
语种英语
WOS记录号WOS:000253039700025
公开日期2010-11-08
内容类型期刊论文
源URL[http://119.78.226.72//handle/331011/11756]  
专题上海天文台_星系宇宙学重点实验室
作者单位1.CAS, Shanghai Astron Observ, Shanghai 200030, Peoples R China
2.USTC, Joint Inst Galaxies & Cosmol, Shanghai, Peoples R China
3.ShAO, Joint Inst Galaxies & Cosmol, Shanghai, Peoples R China
4.Guangzhou Univ, Ctr Astrophys, Guangzhou 510006, Guangdong, Peoples R China
5.Human Normal Univ, Inst Phys, Changsha, Peoples R China
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GB/T 7714
Tao, Jun,Fan, Junhui,Qian, Bochen,et al. Optical monitoring of 3C 390.3 from 1995 to 2004 and possible periodicities in the historical light curve[J]. ASTRONOMICAL JOURNAL,2008,135(2):737-746.
APA Tao, Jun,Fan, Junhui,Qian, Bochen,&Liu, Yi.(2008).Optical monitoring of 3C 390.3 from 1995 to 2004 and possible periodicities in the historical light curve.ASTRONOMICAL JOURNAL,135(2),737-746.
MLA Tao, Jun,et al."Optical monitoring of 3C 390.3 from 1995 to 2004 and possible periodicities in the historical light curve".ASTRONOMICAL JOURNAL 135.2(2008):737-746.
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