Pulsar Models

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Sep 1968

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1968natur.219.1009c&link_type=abstract

Nature, Volume 219, Issue 5158, pp. 1009-1012 (1968).

Physics

6

Scientific paper

A model for pulsars based on vibrating white dwarf stars accounts for a
number of the features of the emissions, and also gives rise to the
possibility of optical fluctuations having a period twice that of the
radio pulses.

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