A summary of radio pulsar polarization

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	A summary of radio pulsar polarization
	Zhu, C.1,2 ; Yan, W.M.1 ; Wang, N.1
	2013
会议名称	3rd Galileo - Xu Guangqi Meeting
会议日期	11-15 Oct. 2011
通讯作者邮箱	na.wang@xao.ac.cn
会议地点	Beijing, China
关键词	Pulsars polarization interstellar medium
卷号	23
页码	174–178
通讯作者	Wang, N.
英文摘要	Pulsars are one of the most polarized radio sources in the universe. Polarization measurements of pulsars provide us a lot of information, not only about the emission process itself, but also about the interstellar medium. This article describes the polarization properties of radio pulsars in general and discusses the observed rotation measure variations with time in pulsars.
收录类别	其他
会议录	International Journal of Modern Physics: Conference Series
会议录出版者	World Scientific Publishing Co. Pte. Ltd., Singapore
语种	英语
ISSN号	2010-1945
内容类型	会议论文
源URL	[http://ir.xao.ac.cn/handle/45760611-7/940]
专题	脉冲星研究团组新疆天文台_射电天文研究室新疆天文台_其它科技计划处
作者单位	1.Xinjiang Astronomical Observatory, Chinese Academy of Sciences 150 Science-1 Street, Urumqi, Xinjiang 830011, China 2.Graduate University of Chinese Academy of Sciences, 19A Yuquan Road Beijing 100049, China
推荐引用方式 GB/T 7714	Zhu, C.,Yan, W.M.,Wang, N.. A summary of radio pulsar polarization[C]. 见:3rd Galileo - Xu Guangqi Meeting. Beijing, China. 11-15 Oct. 2011.