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

Journal of astrophysics and astronomy

N. Wang²  H. G. Wang¹  J. L. Chen1² 

[1] Center for Astrophysics, Guangzhou University, Guangzhou 510006, China.$$;Xinjiang Astronomical Observatory, 150, Science-1 Street, Urumqi, Xinjiang 830011, China.$$

关键词: Pulsar;    emission mechanisms;    phase-resolved spectra.;   

DOI  :  

学科分类：天文学(综合)

来源: Indian Academy of Sciences

【 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 conaldouble pulsars have common `M’-shaped phase-resolved spectra.

【 授权许可】

Unknown