X-Ray Emission from Rotation-Powered Pulsars

Chin. Phys. Lett.

2005, Vol. 22

Issue (4): 1022-1024 DOI:

Original Articles

X-Ray Emission from Rotation-Powered Pulsars

LIN Gui-Fang¹;ZHANG Li^2,1

¹Department of Physics, Yunnan University, Kunming 650031 ²Yunnan Observatory, National Astronomical Observatories, Chinese Academy of Sciences, Kunming 650011

Cite this article:

LIN Gui-Fang, ZHANG Li 2005 Chin. Phys. Lett. 22 1022-1024

Download: PDF(223KB)
Export: BibTeX | EndNote | Reference Manager | ProCite | RefWorks

Abstract We study the properties of pulsed component of hard (2--10keV) x-ray emission from pulsars based on the new version of outer gap model we proposed previously [Astrophys. J. 604(2004)317]. On the frame of this outer gap model, we derive an expression of non-thermal pulsed x-ray luminosity of rotation-powered pulsars, and then apply it to the pulsars whose pulsed x-rays are detected by ASCA. Using the Kolmogorov--Smirnov test, we determine the model parameter. The present results indicate L_X ∝ L^1.15_sd for these x-ray pulsars, which is consistent with the observed data.

Keywords: 97.60.Gb 95.85.Nv 95.85.Pw

Published: 01 April 2005

PACS:	97.60.Gb	(Pulsars)
	95.85.Nv	(X-ray)
	95.85.Pw	(γ-ray)

TRENDMD:

URL:

https://cpl.iphy.ac.cn/ OR https://cpl.iphy.ac.cn/Y2005/V22/I4/01022

Service
	E-mail this article
	E-mail Alert
	RSS
Articles by authors
	LIN Gui-Fang
	ZHANG Li

Related articles from Frontiers Journals

[1]	CAI Yan, A. Taani, WANG Wei, ZHAO Yong-Heng, ZHANG Cheng-Min . Fermi γ-Ray Pulsars: Spectral and Generation Order Parameters**[J]. Chin. Phys. Lett., 2011, 28(8): 1022-1024
[2]	Hasan M. Khan, M. Ismail, K. Khan, P. Akhter . Radioactivity Levels and Gamma-Ray Dose Rate in Soil Samples from Kohistan (Pakistan) Using Gamma-Ray Spectrometry*[J]. Chin. Phys. Lett., 2011, 28(1): 1022-1024
[3]	LIU Xiong-Wei, NA Xue-Sen, XU Ren-Xin, QIAO Guo-Jun . Particle Emission-Dependent Timing Noise of Pulsars**[J]. Chin. Phys. Lett., 2011, 28(1): 1022-1024
[4]	YU Huan, JIANG Ze-Jun,. Multiband Non-Thermal Radiation from the Crab Nebula and the Pulsar Wind Nebula in MSH 15-52[J]. Chin. Phys. Lett., 2010, 27(8): 1022-1024
[5]	K. Khan, A. Jabbar, P. Akhter, M. Tufail, H. M. Khan. Assessment of Primordial Radionuclides in Pakistani Red Bricks and Associated Radiation Doses[J]. Chin. Phys. Lett., 2010, 27(3): 1022-1024
[6]	Shubhra Tiwari, S. N. A. Jaaffrey, Rizwan S. Khan, Sushil K. Gandhi, Santvana Bapna. Timing and Spectral Studies of Pulsar EXO2030+375[J]. Chin. Phys. Lett., 2010, 27(2): 1022-1024
[7]	CHEN Liang, , BAI Jin-Ming, . Is Low-Frequency-Peaked BL Lac Object OJ 287 a TeV Emitter?**[J]. Chin. Phys. Lett., 2010, 27(11): 1022-1024
[8]	WEI Ying-Chun, A. Taani, PAN Yuan-Yue, WANG Jing, CAI Yan, LIU Gao-Chao, LUO A-Li, ZHANG Hong-Bo, ZHAO Yong-Heng . Neutron Star Motion in the Disk Galaxy**[J]. Chin. Phys. Lett., 2010, 27(11): 1022-1024
[9]	LIN Gui-Fang, ZHANG Li. Vacuum Outer-Gap Structure in Pulsar Outer Magnetospheres[J]. Chin. Phys. Lett., 2009, 26(5): 1022-1024
[10]	CHEN Wen-Cong. Evolving into Magnetars from Normal Pulsars with a Low Braking Index[J]. Chin. Phys. Lett., 2009, 26(5): 1022-1024
[11]	ZHOU Ai-Zhi, TAN Jin-Yu, Ali Esamdin, WU Xin-Ji. Two-Component Model for the Interstellar Scattering along the Line of Sight to the Pulsar PSR B0136+57[J]. Chin. Phys. Lett., 2009, 26(12): 1022-1024
[12]	ZHANG Li, WEI Bing-Tao, FANG Jun. Leptonic Origin of TeV Gamma-Ray Emission from Crab Nebula[J]. Chin. Phys. Lett., 2007, 24(10): 1022-1024
[13]	CHEN Shi-Bo, ZHANG Li,. One-Dimensional Electric Field Structure of an Outer Gap Accelerator[J]. Chin. Phys. Lett., 2006, 23(10): 1022-1024
[14]	LIU Dang-Bo, CHEN Lei, LING Jia-Jie, YOU Jun-Han. Matching Condition in γ-γ Annihilation Absorption[J]. Chin. Phys. Lett., 2005, 22(6): 1022-1024
[15]	JIANG Ze-Jun, ZHANG Li,. Effect of Gamma-Ray Beaming on the Fluxes of Gamma-Ray Pulsars[J]. Chin. Phys. Lett., 2005, 22(5): 1022-1024

Viewed

Full text

Abstract