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

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

Jun 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011japa...32..333c&link_type=abstract

Journal of Astrophysics and Astronomy, Volume 32, Issue 1-2, pp. 333-335

Astronomy and Astrophysics

Astrophysics

Pulsar, Emission Mechanisms, Phase-Resolved Spectra

Scientific paper

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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