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

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    • Keywords


      Pulsar; emission mechanisms; phase-resolved spectra.

    • Abstract


      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.

    • Author Affiliations


      J. L. Chen1 2 H. G. Wang3 N. Wang1

      1. Xinjiang Astronomical Observatory, 150, Science-1 Street, Urumqi, Xinjiang 830011, China.
      2. Graduate University of the Chinese Academy of Scienes, 19A Yuquan Road, Beijing 100049, China.
      3. Center for Astrophysics, Guangzhou University, Guangzhou 510006, China.
    • Dates

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