Timing Irregularities and the Neutron Star Stability

Details Timing Irregularities and the Neutron Star Stability Timing Irregularities and the Neutron Star Stability

Aug 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006iaujd...2e..14u&link_type=abstract

On the Present and Future of Pulsar Astronomy, 26th meeting of the IAU, Joint Discussion 2, 16-17 August, 2006, Prague, Czech Re

Astronomy and Astrophysics

Astronomy

Scientific paper

Observations show that the different manifestations of neutron stars exhibit measurable departures from the predicted slow down. This has been largely attributed to rotational irregularities - timing noise, glitches, and precession. Here, We present an analysis of the regular spin-down and jump parameters for a combined set of the pulsars (radio, optical, x-ray and gamma-ray) and magnetars. We attempt to quantify the stability of neutron stars, in general.

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