期刊文献+

Infrared Polarization and Beaming Effect for BL Lac Objects

下载PDF
导出
摘要 With the idea of the beaming models,we derive a relation between the observed polarization and Doppler-corrected magnitude,that is,the observed polarization is in anti-correlation with the Doppler-corrected magnitude.Making use of the infrared data observed simultaneously by Impey et al.[Mon.Not.R.Astron.Soc.200(1982)19;209(1984)245]and Holmes et al.[ibid.210(1984)961]we found that(1)there is a significant correlation between the observed maximum polarization and Doppler-corrected magnitude but the polarization is not in anti-correlation with the Doppler corrected magnitude;(2)the maximum infrared polarization is strongly correlated with the maximum optical polarization.Our conclusion is that the infrared polarization depends only on the degree of ordering of the magnetic field in the synchotron emission regions and not on the beaming effect.Both infrared and optical emissions originate from the synchrotron radiation.
作者 MEI Dong-Cheng XIE Guang-Zhong 梅冬成;谢光中(Yunnan Astronomical Observatory,Chinese Academy of Sciences,Kunming 650011;The National Astronomical Observatories,Chinese Academy of Sciences;Yunnan Astrophysics Center,Yunnan University,Kunming 650091)
出处 《Chinese Physics Letters》 SCIE CAS CSCD 2001年第5期708-710,共3页 中国物理快报(英文版)
基金 Supported by the National Natural Science Foundation of China under Grant No.19863001 the Natural Science Foundation of Yunnan Province(Grant No.98A010M)。
  • 相关文献

相关作者

内容加载中请稍等...

相关机构

内容加载中请稍等...

相关主题

内容加载中请稍等...

浏览历史

内容加载中请稍等...
;
使用帮助 返回顶部