Phase-Resolved Spectra of PSR B0525+21 and PSR B2020+28

被引：0
|
作者：
J. L. Chen
H. G. Wang
N. Wang
机构：
[1] Xinjiang Astronomical Observatory,Center for Astrophysics
[2] Graduate University of the Chinese Academy of Scienes,undefined
[3] Guangzhou University,undefined
来源：
Journal of Astrophysics and Astronomy | 2011年 / 32卷
关键词：
Pulsar; emission mechanisms; phase-resolved spectra;
D O I：
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中图分类号：
学科分类号：
摘要：
Using the published data of multi-frequency time-aligned pulse profiles from Kuzmin et al. (1998), we calculate the phase-resolved spectra of PSRs B0525+21 and B2020+28. The results reveal that conal-double pulsars have common ‘M’-shaped phase-resolved spectra.
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