Historic light curve and long-term optical variation of BL Lacertae 2200+420

被引:132
作者
Fan, JH
Xie, GZ
Pecontal, E
Pecontal, A
Copin, Y
机构
[1] Observ Lyon, Ctr Rech Astron Lyon, F-69563 St Genis Laval, France
[2] Guangzhou Normal Univ, Ctr Astrophys, Guangzhou 510400, Peoples R China
[3] Chinese Acad Sci, Joint Lab Opt Astron, Beijing 100864, Peoples R China
[4] Chinese Acad Sci, Yunnan Observ, Kunming 650011, Peoples R China
关键词
BL Lacertae objects : individual (2200+420);
D O I
10.1086/306301
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
In this paper, historical optical (UBVRI) data and newly observed data from the Yunnan Observatory of China (over similar to 100 yr) are presented for BL Lacertae. Large variations of Delta U = 5.12 mag, Delta B = 5.31 mag, Delta V = 4.73 mag, Delta R = 2.59 mag, and Delta I = 2.54 mag, and color indices of U-B = -0.11 +/- 0.20, B-V = 1.0 +/- 0.11, V - R = 0.73 +/- 0.19, V - I = 1.42 +/- 0.25, R - I = 0.82 +/- 0.11, and B - I = 2.44 +/- 0.29 have been obtained from the literature. The Jurkevich method is used to investigate the existence of periods in the B-band light curve, and a long-term period of 14 yr is found. The 0.6 and 0.88 yr periods reported by Webb et al. are confirmed. In addition, a close relation between B - I and B is found, suggesting that the spectrum flattens when the source brightens.
引用
收藏
页码:173 / 178
页数:6
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