Phase-Resolved Spectra of PSR B0525+21 and PSR B2020+28
Using the published data of multi-frequency timealigned 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.
J.L.Chen H.G.Wang N.Wang
Xinjiang Astronomical Observatory,150,Science-1 Street,Urumqi,Xinjiang 830011,China Graduate Univers Center for Astrophysics,Guangzhou University,Guangzhou 510006,China Xinjiang Astronomical Observatory,150,Science-1 Street,Urumqi,Xinjiang 830011,China
国际会议
International Conference of Multiwavelength Variability of Blazars(Blazar多波段光变国际学术会议)
广州
英文
333-335
2010-09-20(万方平台首次上网日期,不代表论文的发表时间)