Rotational Properties of Neutron Star Models

Details Rotational Properties of Neutron Star Models Rotational Properties of Neutron Star Models

Nov 1969

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1969natur.224..566c&link_type=abstract

Nature, Volume 224, Issue 5219, pp. 566-567 (1969).

Physics

9

Scientific paper

IT has been suggested that pulsars are rotating neutron
stars1 and that the energy source of the Crab nebula is the
loss of rotational energy from the Crab pulsar2. Because
neutron stars are quite dense, general relativistic effects are large
and cannot be neglected.

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