Studying Pulsar Emission Regions Using Interstellar Scattering

Details Studying Pulsar Emission Regions Using Interstellar Scattering Studying Pulsar Emission Regions Using Interstellar Scattering

Oct 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001ap%26ss.278...65g&link_type=abstract

Astrophysics and Space Science, v. 278, Issue 1/2, p. 65-70 (2001).

Astronomy and Astrophysics

Astrophysics

1

Scientific paper

Radio-wave scattering in the interstellar plasma provides the means to circumvent the diffraction limit for earth-based instruments, and to image the emission regions of pulsars. For the past 25 years, observers have sought to exploit this fact to learn how pulsars shine. I review the techniques developed, and summarize measurements of size of emission regions of pulsars to date.

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