Mode switching and subpulse drifting in PSR B0826-34
Ali EsamdinUrumqi Observatory, National Astronomical Observatories, CAS, 40 South Beijing Road, Urumqi 830011, ChinaA. G. LyneUniversity of Manchester, Jodrell Bank Observatory, Macclesfield, Cheshire, SK 11 9DLFrancis Graham-SmithUniversity of Manchester, Jodrell Bank Observatory, Macclesfield, Cheshire, SK 11 9DLM. KrämerUniversity of Manchester, Jodrell Bank Observatory, Macclesfield, Cheshire, SK 11 9DLR. N. ManchesterAustralia Telescope National Facility, CSIRO, PO Box 76 Epping, NSW 1710, AustraliaX. WuDepartment of Astronomy, Peking University, Beijing 100871, China
2004en
ABI
Annotatsiya
PSR B0826−34 (PSR J0828−3417) is known as a pulsar whose emission extends through the whole pulse period (P = 1.848 sec). It is a relatively old pulsar with a characteristic age of 3×10 7 yr. PSR B0826−34 exhibits some extreme
Hali tarjima qilinmagan
Identifikatorlar
Iqtiboslar va manbalar
2 ta iqtibos0 ta foydalanilgan manba