thevariabilityofbllac3c66a
文献类型：期刊论文
| 作者 | Su Chengyue |
| 刊名 | chinesephysics
 |
| 出版日期 | 2004 |
| 卷号 | 13期号:8页码:1375 |
| ISSN号 | 1009-1963 |
| 英文摘要 | It is now known that there are supermassive black holes at the centre of a galaxy, surrounded by an accretion disc. The black hole-jet-accretion disc model plays an important role in the explanation of the observational properties of active galactic nuclei. BL Lacertae objects form a subclass of blazars; they are monitored through electromagnetic wave bands. During the OJ-94 project, 3C 66A was observed as a comparison object of OJ287 and found to display a possible 65-day period in the V light curve. In this paper, we show that the instability of an accretion disc surrounding a massive central black hole (2.5 x 10(7)Mcircle dot) may explain this period in 3C 66A. |
| 语种 | 英语 |
| 源URL | [http://ir.bao.ac.cn/handle/114a11/50735]  |
| 专题 | 中国科学院国家天文台 |
| 作者单位 | 中国科学院国家天文台 |
| 推荐引用方式 GB/T 7714 | Su Chengyue. thevariabilityofbllac3c66a[J]. chinesephysics,2004,13(8):1375. |
| APA | Su Chengyue.(2004).thevariabilityofbllac3c66a.chinesephysics,13(8),1375. |
| MLA | Su Chengyue."thevariabilityofbllac3c66a".chinesephysics 13.8(2004):1375. |
入库方式： OAI收割
来源：国家天文台
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