Long-Term Optical Spectra Variability of BL Lacertae Object S5 0716+714
Based on the long-term data from observations, we present an evidence for its spectral index variability behaviour in optical bands for BL Lacertae object S5 0716+714. We find that the spectral index variability period is in agreement with the flux variability period of about 1180 days in optical bands. We also find that the spectral index variability has periods of about 71 and 60 days which cannot be compared with the amplitude of longterm variability.
Zhang Hao Jing Zhao Gang Zhang Xiong Bai Jing Ming Tang Ling Xu Yun Bing
College of Physics and Electronics,Yunnan Normal University,Kunming 650092,China Yunnan Astronomical National Astronomical Observatories,Chinese Academy of Sciences,Beijing 100012,China College of Physics and Electronics,Yunnan Normal University,Kunming 650092,China Yunnan Astronomical Observatory,National Astronomical Observatories,Chinese Academy of Sciences,Kunm
国际会议
International Conference of Multiwavelength Variability of Blazars(Blazar多波段光变国际学术会议)
广州
英文
131-135
2010-09-20(万方平台首次上网日期,不代表论文的发表时间)