Evidence on neutron star structure from pulsars and related objects

Details Evidence on neutron star structure from pulsars and related objects Evidence on neutron star structure from pulsars and related objects

Jan 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976ap%26ss..39....3r&link_type=abstract

(Symposium on Solid State Astrophysics, University College, Cardiff, Wales, July 9-12, 1974.) Astrophysics and Space Science, vo

Astronomy and Astrophysics

Astrophysics

1

Neutron Stars, Pulsars, Stellar Magnetic Fields, Stellar Mass, Stellar Structure, X Ray Sources, Binary Stars, Moments Of Inertia, Rigidity, Stellar Rotation

Scientific paper

A brief summary is presented of those properties of pulsars and binary X-ray sources that seem most directly relevant to the actual structure of neutron stars and the effects of ultrastrong magnetic fields. The discussion focuses on mass determinations for the X-ray sources Her X-1 and Cen X-3, estimates of the moments of inertia of the Crab pulsar and the pulsar JP 1953, and studies of pulsar surface magnetic fields. Other properties mentioned include the rigidity of a neutron star's crust, seismic activity (glitches, crustquakes, and microquakes), and pulsar wobble (similar in some ways to free precession).-

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