Mildly Recycled Pulsars at High-Energies

Details Mildly Recycled Pulsars at High-Energies Mildly Recycled Pulsars at High-Energies

Aug 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011aipc.1357..261p&link_type=abstract

RADIO PULSARS: AN ASTROPHYSICAL KEY TO UNLOCK THE SECRETS OF THE UNIVERSE. AIP Conference Proceedings, Volume 1357, pp. 261-264

Astronomy and Astrophysics

Astrophysics

Neutron Stars, Gamma-Ray Production, Time Series, X-Ray Binary Stars, Neutron Stars, Gamma-Ray Sources, Gamma-Ray Bursts, Time Series Analysis, Time Variability, X-Ray Binaries

Scientific paper

Mildly recyled pulsars (MRP), conventionally defined as neutron star having spin period in the 20-100 ms range and surface magnetic field <1011 Gauss, probably rise from binary systems (disrupted or not) with an intermediate or an high mass companion. Despite their relatively low spin-down energies compared to the ``fully'' recycled millisecond pulsars (arising from common low mass X-ray binaries), nearby MRPs can be detected by deep X-ray observations and by timing analysis of the very long data span provided by gamma-ray space detectors. The discovery of peculiar timing and spectral properties, possibly transitional, of the MRPs can be of the utmost importance to link different classes of neutron stars and study their evolution.

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