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Mean pulse analysis and spectral character study of pulsar PSR B2111+46 被引量:6

Mean pulse analysis and spectral character study of pulsar PSR B2111+46
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摘要 PSR B2111+46 is studied and analyzed by the method of Gaussian fit separation of the average profile (GFSAP). It has been observed at six frequencies,408, 610, 925, 1408, 1640, and 4850 MHz, serving as an excellent sample for a multifrequency analysis. Applying the GFSAP method we find that PSR B2111+46 hasfive components in its profile at all six frequencies. The result supports Rankin's 'core-double cone' model in emission region. On the basis of component decomposition, we discuss the geometrical structure of core, inner cone and outer cone, the emission beam radius, the emission region altitude and the geometry symmetry. We also examine the spectrum characteristics of core, inner cone and outercone. It is found that the spectrum of the core is steeper than the inner and outer cone. PSR B2111+46 is studied and analyzed by the method of Gaussian fit separation of the average profile (GFSAP). It has been observed at six frequencies, 408, 610, 925, 1408, 1640, and 4850 MHz, serving as an excellent sample for a multifrequency analysis. Applying the GFSAP method we find that PSR B2111+46 has five components in its profile at all six frequencies. The result supports Rankin’s “core-double cone” model in emission region. On the basis of component decomposition, we discuss the geometrical structure of core, inner cone and outer cone, the emission beam radius, the emission region altitude and the geometry symmetry. We also examine the spectrum characteristics of core, inner cone and outer cone. It is found that the spectrum of the core is steeper than the inner and outer cone.
出处 《Science China(Physics,Mechanics & Astronomy)》 SCIE EI CAS 2003年第1期104-112,共9页 中国科学:物理学、力学、天文学(英文版)
基金 国家自然科学基金,the United Astronomy Laboratory of CAS
关键词 pulsars COMPONENT decomposition EMISSION region. pulsars component decomposition emission region
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  • 10Kuzmin,A.D,Losovsky,B.Y.Unusual frequency dependence of the integrated profile of the millisecond pulsar PSR J2145-0705[].A&A.1996

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