Abstract
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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RADHAKRISHNAN, V., COOKE, D., KOMESAROFF, M. et al. Evidence in Support of a Rotational Model for the Pulsar PSR 0833–45. Nature 221, 443–446 (1969). https://doi.org/10.1038/221443a0
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DOI: https://doi.org/10.1038/221443a0
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