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Thirteen drift bands in PSR B0826-34
A.Esamdin1; A.G.Lyne2; M.Kramer2; F.Graham-Smith2; R.N.Manchester3
2004
Conference Name218th Symposium of the International-Astronomical-Union on Yound Neutron Stars and Their Environments
Source PublicationYOUNG NEUTRON STARS AND THEIR ENVIRONMENTS
Volume218
Pages341-342
Conference Date2003-07-14
Conference PlaceSydney, AUSTRALIA
PublisherAstronomical Society of the Pacific
Contribution Rank1
Abstract

By developing a new technique, 13 drifting subpulses have been revealed across one period in PSR B0826-34. The variation of drift rate when drifting subpulses drift through different longitude regions are noticed. A weak emission mode was detected during its apparent null.

Funding OrganizationIAU ; IAU
KeywordPulsar
Subject Area致密天体、高能和基础物理
Indexed ByCPCI
Funding Project脉冲星研究团组
Language英语
ISSN0074-1809
WOS IDWOS:000227426000088
Citation statistics
Cited Times:1[WOS]   [WOS Record]     [Related Records in WOS]
Document Type会议论文
Identifierhttp://ir.xao.ac.cn/handle/45760611-7/283
Collection射电天文研究室_脉冲星研究团组
光学天文与技术应用研究室
Corresponding AuthorA.Esamdin
Affiliation1.National Astronomical Observatories/Urumgi Observatory, CAS Urumgi 830011,P.R. China
2.University of Manchester,Jodrell Bank Observatory,Macclesfield, Cheshire SK11 9DL,UK
3.Australia Telescope National Facility, CSIRO,P.O. Boz 76, Epping NSW 1710, Australia
First Author AffilicationXinjiang Astronomical Observatory, Chinese Academy of Sciences
Corresponding Author AffilicationXinjiang Astronomical Observatory, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
A.Esamdin,A.G.Lyne,M.Kramer,et al. Thirteen drift bands in PSR B0826-34[C]:Astronomical Society of the Pacific,2004:341-342.
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