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Volumn 33, Issue 4, 2004, Pages 592-596

Phase-coherent timing of PSR J1811-1925: The pulsar at the heart of G11.2-0.3

Author keywords

G11.2 0.3; Phase coherent timing; PSR J1811 1925; Pulsar

Indexed keywords

ASTRONOMY; BRAKING; ENERGY ABSORPTION; GAMMA RAYS; LIGHT EMISSION; PHOTONS; TIME MEASUREMENT;

EID: 1842741151     PISSN: 02731177     EISSN: None     Source Type: Journal    
DOI: 10.1016/j.asr.2003.07.028     Document Type: Article
Times cited : (9)

References (24)
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  • 16
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    • Spin-down of an oblique rotator with a current starved outer magnetosphere
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  • 17
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    • Murray, S.S.1    Slane, P.O.2    Seward, F.D.3    Ransom, S.M.4    Gaensler, B.M.5
  • 18
    • 0036605492 scopus 로고    scopus 로고
    • Re-examining the X-ray versus spin-down luminosity correlation of rotation powered pulsars
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  • 21
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    • Discovery of a 65 ms pulsar in the supernova remnant G11.2-0.3 with ASCA
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    • Detection of a hard X-ray plerion in the candidate historical remnant G11.2-0.3
    • Vasisht G. Aoki T. Dotani T. Kulkarni S.R. Nagase F. Detection of a hard X-ray plerion in the candidate historical remnant G11.2-0.3 Astrophys. J. 456 1996 L59-L62
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    • A phase-connected braking index measurement for the Large Magellanic Cloud pulsar PSR B0540-69
    • Zhang W. Marshall F.E. Gotthelf E.V. Middleditch J. Wang Q.D. A phase-connected braking index measurement for the Large Magellanic Cloud pulsar PSR B0540-69 Astrophys. J. 554 2001 L177-L180
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* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.