BL Lac天体S50716+714的光变周期特性研究  

A study of the light curve periodic behavior of BL Lac object S5 0716+714

作　　者：张皓晶[1] 张雄[2] 

机构地区：[1]中国科学院国家天文台,北京100012 [2]云南师范大学物理系,昆明650092

出　　处：《物理学报》2007年第7期4305-4311,共7页Acta Physica Sinica

基　　金：国家自然科学基金项目(批准号:10363002和10663002)资助的课题.~~

摘　　要：从大量文献资料中,收集了BLLac天体S50716+714光学B,V,R,I波段的有效观测数据点共16818个,获得了从1994年至2006年的长期光变曲线,光变曲线表明S50716+714天体存在完整的非正弦变化并且它的活动非常剧烈.用功率谱方法分析了S50716+714天体的光变周期,结果表明S50716+714天体存在的长光变周期为1.1年,Raiteri等人发现的3.3年周期可能是1.1年周期的叠合.预期在2007年2月应该为S50716+714天体的再次爆发期.From a large volume of literature we have collected a total of 16818 datapoints of effective observation of BL Lae object S5 0716 ＋ 714 in the optical band, and constructed its long-term light curve from 1994 to 2006 AD. The light curve shows that S5 0716 ＋ 714 is very active and exhibits very complicated non-sinusoidal variations. We used power spectrum method to analyze the period of light curve variation. Our results show that the long-term period of variation is 1.1 year. Time of coincidence is possible, Raiteri et al. have found the period of 3.3 year, which may be a multiple of 1.1-year periods. We expect next burst in 2006 July.

关 键 词：BL Lac天体S5 0716+714 光变周期 功率谱方法 

分 类 号：P141[天文地球—天体物理]