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Young Pulsars from the Parkes Multibeam Pulsar Survey and their Associations | | R.N.Manchester
; J.F.Bell
; F.Camilo
; M.Kramer
; A.G.Lyne
; G.B.Hobbs
; B.C.Joshi
; F.Crawford
; N.D’Amico
; A.Possenti
; V.M.Kaspi
; I.H.Stairs
; | | Date: |
7 Dec 2001 | | Subject: | astro-ph | | Affiliation: | ATNF-CSIRO), F.Camilo (Columbia), M.Kramer, A.G.Lyne, G.B.Hobbs, B.C.Joshi (Jodrell Bank), F.Crawford (Lockeed), N.D’Amico, A.Possenti (Bologna), V.M.Kaspi (McGill), I.H.Stairs (NRAO-GB | | Abstract: | The Parkes multibeam pulsar survey is covering a 10deg-wide strip of the southern Galactic plane from l=260deg to l=50deg. It utilizes a 13-beam receiver operating in the 20-cm band on the Parkes 64-m radio telescope and is much more sensitive than any previous large-scale survey. Most of the 608 pulsars discovered so far are relatively distant and many are young, with 37 having a characteristic age of less than 10^5 years. At least one of these is associated with a supernova remnant and four other probable associations are suggested. Several multibeam pulsars have high values of the parameter Edot/d^2 and are within the position error contours of unidentified EGRET gamma-ray sources. These possible associations will be tested with the advent of new gamma-ray telescopes. | | Source: | arXiv, astro-ph/0112166 | | Services: | Forum | Review | PDF | Favorites | |
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