Evidence in Support of a Rotational Model for the Pulsar PSR 0833-45

Details Evidence in Support of a Rotational Model for the Pulsar PSR 0833-45 Evidence in Support of a Rotational Model for the Pulsar PSR 0833-45

Feb 1969

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1969natur.221..443r&link_type=abstract

Nature, Volume 221, Issue 5179, pp. 443-446 (1969).

Physics

81

Scientific paper

Measurements of the pulsar tentatively identified with the supernova
remnant Vela X support the rotational model. This pulsar is remarkable
for the very high degree of linear polarization in its signals.

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