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FERMI STUDY OF gamma-RAY MILLISECOND PULSARS: THE SPECTRAL SHAPE AND PULSED EMISSION FROM J0614-3329 UP TO 60 GeV
Xing, Yi; Wang, Zhongxiang
刊名ASTROPHYSICAL JOURNAL
2016-11-10
卷号831期号:2
关键词Gamma Rays: Stars Pulsars: General Pulsars: Individual (Psr J0614-3329)
ISSN号0004-637X
DOI10.3847/0004-637X/831/2/143
英文摘要We report our analysis of the Fermi Large Area Telescope data for 39 millisecond pulsars (MSPs) listed in the second gamma-ray pulsar catalog. Spectra of the pulsars are obtained. We fit the spectra with a function of a power law with exponential cutoff, and find the best-fit parameters of photon index T = 1.54(-0.11)(+0.10) and cutoff energy E-c = 3.70(-0.70)(+0.95) GeV. This spectral shape, which includes the intrinsic differences in the spectra of the MSPs, can be used for finding candidate MSPs and unidentified types of sources detected by Fermi at high Galactic latitudes. In one of the MSPs, PSR J0614-3329, we find significant pulsed emission up to 60 GeV. The result has thus added this MSP to the group of pulsars that have been detected with pulsed emission at. energies of tens of GeV. Comparing the gamma-ray spectrum of PSR. J0614-3329 with those of the Crab and Vela pulsars, we discuss possible emission mechanisms for the very high-energy component.
WOS研究方向Astronomy & Astrophysics
语种英语
出版者IOP PUBLISHING LTD
WOS记录号WOS:000400474300007
内容类型期刊论文
源URL[http://119.78.226.72/handle/331011/32597]  
专题中国科学院上海天文台
通讯作者Xing, Yi
作者单位Chinese Acad Sci, Shanghai Astron Observ, Key Lab Res Galaxies & Cosmol, 80 Nandan Rd, Shanghai 200030, Peoples R China
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Xing, Yi,Wang, Zhongxiang. FERMI STUDY OF gamma-RAY MILLISECOND PULSARS: THE SPECTRAL SHAPE AND PULSED EMISSION FROM J0614-3329 UP TO 60 GeV[J]. ASTROPHYSICAL JOURNAL,2016,831(2).
APA Xing, Yi,&Wang, Zhongxiang.(2016).FERMI STUDY OF gamma-RAY MILLISECOND PULSARS: THE SPECTRAL SHAPE AND PULSED EMISSION FROM J0614-3329 UP TO 60 GeV.ASTROPHYSICAL JOURNAL,831(2).
MLA Xing, Yi,et al."FERMI STUDY OF gamma-RAY MILLISECOND PULSARS: THE SPECTRAL SHAPE AND PULSED EMISSION FROM J0614-3329 UP TO 60 GeV".ASTROPHYSICAL JOURNAL 831.2(2016).
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