Nanoarcsecond Structure of the VELA Pulsar via Interstellar Scattering

Details Nanoarcsecond Structure of the VELA Pulsar via Interstellar Scattering Nanoarcsecond Structure of the VELA Pulsar via Interstellar Scattering

May 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998aas...192.4607g&link_type=abstract

American Astronomical Society, 192nd AAS Meeting, #46.07; Bulletin of the American Astronomical Society, Vol. 30, p.879

Astronomy and Astrophysics

Astronomy

Scientific paper

We study the radio emission region of the Vela pulsar at nanoarcsecond angular resolution, using scattering in the Vela supernova remnant as an AU-scale lens. We present results of interferometric observations with ground-based radiotelescopes and the HALCA orbiting radiotelescope, and the resulting picture of the pulsar's emission region. We suggest that radio-wave refraction within the pulsar's magnetosphere may explain this structure.

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