Pulsars, AXPs and SGRs

Details Pulsars, AXPs and SGRs Pulsars, AXPs and SGRs

May 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001aipc..565..305m&link_type=abstract

YOUNG SUPERNOVA REMNANTS: Eleventh Astrophysics Conference. AIP Conference Proceedings, Volume 565, pp. 305-314 (2001).

Astronomy and Astrophysics

Astrophysics

3

Supernova Remnants, Pulsars, X-Ray Sources, X-Ray Bursts, Neutron Stars

Scientific paper

Pulsars, including both those detected at radio wavelengths and those only detectable at high energies, Anomalous X-ray pulsars (AXPs) and Soft Gamma-ray Repeaters (SGRs) are all believed to be rotating neutron stars. Yet they have very different properties. In the past few years the number of known objects in all of these classes has increased dramatically. Many of these new discoveries are young neutron stars, leading to a significant increase in the number of believable associations with supernova remnants. In this review, I outline the main properties of each class of object and describe some recent results. .

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