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XBLs和RBLs间的光度与宽波段谱指数的相关性分析 被引量:1

The Correlation Between Broad-band Spectral Index and Luminosity for XBLs and RBLs
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摘要 对Fossati等人的研究中所给出的Blazar样本分别计算从射电到X射线波段的光度、宽波段光谱指数. 在此基础上研究了XBLs和RBLs间的光度与宽波段谱指数的相关性质. 结果表明:XBLs和RBLs之间存在着较强的相关性质,XBLs和RBLs位于不同的区域,可以通过0.75rxa=较好的区分开来,这意味着它们之间的能谱分布形状是有差异的因而有助于我们了解的其内部辐射机制,最后对结果进行讨论. Using the sample of XBLs and RBLs presented by Fossati et al.(1998), we calculated the broad-band spectral index and luminosity from radio to X-ray of each source respectively. We also made a statistical analysis between broad-band spectral index and luminosity for XBLs and RBLs. The main results are as follows: XBLs and RBLs can be separated by the value 0.75rxa=. There are very strong correlations between broad-band spectral index and luminosity between XBLs and RBLs. It is helpful for us to understand the radiation mechanism for these different kinds of blazars.
作者 丁世学
出处 《襄樊学院学报》 2004年第5期10-14,共5页 Journal of Xiangfan University
基金 湖北省教育厅重点科研项目(2003A001)
关键词 BLAZARS 光度 谱能分布 非热辐射 Blazars Luminosity SEDs Non thermal radiation
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参考文献7

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同被引文献8

  • 1丁世学.XBLs和平谱射电类星体间峰值频率与光谱指数的相关性分析[J].华中师范大学学报(自然科学版),2004,38(4):430-432. 被引量:2
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  • 3Giommi P, Barr P, Garilli B,et al. A study of BL Lacertaetype objects with Exosat. I-Flux correlations, luminosity variability, and spectral variability[J]. APJ, 1990, 356:432-455.
  • 4Giommi P, Padovani P. BL-Lacertae Reunification[J]. MNRAS, 1994, 268: L51-L54.
  • 5Padovani P, Giommi P. The connection between x-ray- and radio-selected BL Lacertae objects [J]. APJ, 1995, 444:567-581.
  • 6Fossati G, Maraschi L, Celotti A, et al. A unifying view of the spectral energy distributions of blazers[J]. MNRAS,1998, 299: 433-448.
  • 7Mei D C, Zhang L, Jiang Z J. Radio luminosities and classificatory criteria of BL Lacertae objects[J]. A&A, 2002,391:917-922.
  • 8Sambruna R M, Maraschi L, Urry C M. On the Spectral Energy Distributions of Blazars[J]. APJ, 1996, 463:444-456.

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