Recent discoveries of energetic young radio pulsars

Astrophysics, abstract
astro-ph/0301327

From: Dunc Lorimer <drl@jb.man.ac.uk>

Date: Thu, 16 Jan 2003 16:30:07 GMT   (369kb)

Authors:
D.R. Lorimer (Jodrell Bank Observatory)

Comments: 10 pages, 5 figures, to appear in the proceedings of the workshop
“Pulsars, AXPs and SGRs observed with BeppoSAX and other Observatories” held
in Marsala, Sicily, September 2001

The observed population of young radio pulsars has grown substantially in
recent years due to a combination of large-scale surveys and deep targeted
searches. Many of the pulsars are associated with supernova remnants and/or
unidentified gamma-ray sources. This review summarises the state of play and
looks ahead to likely advances in the near future.

References and citations for this submission:

SLAC-SPIRES HEP (refers to ,
cited by, arXiv reformatted)