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Volumn 337, Issue 6097, 2012, Pages 946-949

Absorption features in the X-ray spectrum of an ordinary radio pulsar

Author keywords

[No Author keywords available]

Indexed keywords

ABSORPTION; NUMERICAL MODEL; SPECTRAL ANALYSIS; X-RAY;

EID: 84865281093     PISSN: 00368075     EISSN: 10959203     Source Type: Journal    
DOI: 10.1126/science.1221378     Document Type: Article
Times cited : (50)

References (27)
  • 9
    • 84922700018 scopus 로고    scopus 로고
    • A simpler model, BB+PL, does not produce a satisfactory fit
    • A simpler model, BB+PL, does not produce a satisfactory fit.
  • 10
    • 84922757058 scopus 로고    scopus 로고
    • note
    • This NH value is used in all the subsequent phase-resolved spectral fits because having NH tied and fitting for it in the phase-resolved spectra results in a similar but more uncertain value.
  • 11
    • 0041887624 scopus 로고    scopus 로고
    • W. Becker, H. Lesch, J. Trümper, Eds. Max-Plank-Institut für Extraterrestrische Physik, Garching, Germany
    • G. G. Pavlov, V. E. Zavlin, D. Sanwal, in Neutron Stars, Pulsars, and Supernova Remnants, W. Becker, H. Lesch, J. Trümper, Eds. (Max-Plank-Institut für Extraterrestrische Physik, Garching, Germany, 2002), pp. 273-286.
    • (2002) Neutron Stars, Pulsars, and Supernova Remnants , pp. 273-286
    • Pavlov, G.G.1    Zavlin, V.E.2    Sanwal, D.3


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.