中文

耀变体 W2R 1926+42 中混沌的搜寻及其可能后果

高能天体物理现象 2016-03-02 v1 星系天体物理

摘要

我们在 KeplerKepler 视场耀变体 W2R 1926+42 的光变曲线中搜寻低维混沌特征。我们的分析采用了常用的关联积分法。我们发现光变曲线中不存在低维混沌的明显证据。若进一步证实,这些结果对建立耀变体辐射机制模型可能具有重要意义。

关键词

引用

@article{arxiv.1603.00140,
  title  = {A search for chaos in the blazar: W2R 1926+42 and its possible consequence},
  author = {Banibrata Mukhopadhyay and Rumen Bachev and Anton Strigachev},
  journal= {arXiv preprint arXiv:1603.00140},
  year   = {2016}
}

备注

6 pages including 3 figures; to appear in the Proceedings of 14th Marcel Grossman Meeting (MG14), Rome, Italy, 12-18 July 2015; based on the talk given in the meeting in the session GN2