The Parkes Multibeam Pulsar Survey - II. Discovery and timing of 120 pulsars

被引:154
作者
Morris, DJ [1 ]
Hobbs, G
Lyne, AG
Stairs, IH
Camilo, F
Manchester, RN
Possenti, A
Bell, JF
Kaspi, VM
Amico, ND
McKay, NPF
Crawford, F
Kramer, M
机构
[1] Univ Manchester, Jodrell Bank Observ, Macclesfield SK11 9DL, Cheshire, England
[2] Natl Radio Astron Observ, Green Bank, WV 24944 USA
[3] Columbia Univ, Columbia Astrophys Lab, New York, NY 10027 USA
[4] CSIRO, Australia Telescope Natl Facil, Epping, NSW 1710, Australia
[5] Osservatorio Astron Bologna, I-40127 Bologna, Italy
[6] MIT, Ctr Space Res, Cambridge, MA 02139 USA
[7] McGill Univ, Dept Phys, Montreal, PQ H3A 2T8, Canada
[8] Cagliari Astron Observ, I-09012 Capoterra, Ca, Italy
[9] Haverford Coll, Dept Phys, Haverford, PA 19041 USA
基金
美国国家科学基金会;
关键词
methods : observational; pulsars : general; pulsars : individual : PSR J1734-3333; pulsars : individual : PSR J1830-1135;
D O I
10.1046/j.1365-8711.2002.05551.x
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The Parkes Multibeam Pulsar Survey is a sensitive survey of a strip of the Galactic plane with \b\ < 5degrees and 260degrees < l < 50degrees at 1374 MHz. Here we report the discovery of 120 new pulsars and subsequent timing observations, primarily using the 76-m Lovell radio telescope at Jodrell Bank. The main features of the sample of 370 published pulsars discovered during the multibeam survey are described. Furthermore, we highlight two pulsars: PSR J1734-3333, a young pulsar with the second highest surface magnetic field strength among the known radio pulsars, B (s)= 5.4 x 10(13)G, and PSR J1830-1135, the second slowest radio pulsar known, with a 6-s period.
引用
收藏
页码:275 / 290
页数:16
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