FREQUENCY DEPENDENCE OF POLARIZATION OF PULSAR CP 0328

被引:2
作者
GOLDSTEIN, SJ
机构
[1] Department of Astronomy, University of Virginia, Box 3818, Charlottesville
关键词
D O I
10.1126/science.163.3869.810
中图分类号
O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];
学科分类号
07 ; 0710 ; 09 ;
摘要
The circularly polarized emission from the pulsar CP 0328 has an approximately flat spectrum in the 1-megahertz band centered at 113.6 megahertz, whereas the linearly polarized emission varies with frequency and from pulse to pulse. A simple model for the source that has a constant Faraday rotation measure fits some of the linearly polarized spectra observed for individual pulses, but changes in the rotation measure of as much as 30 radians per square meter are required between adjacent pulses. The simple model does not fit the average spectrum of the linearly polarized emission, although the average spectrum had the same form on two nights.
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页码:810 / +
页数:1
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