Intensities of Inverse Compton Gamma-Rays in Galactic Medium Latitude

Zhang Li

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《中国物理C》（英文）编辑部

2024年10月30日

Chinese Physics C> 1995, Vol. 19> Issue(11) : 974-979

Intensities of Inverse Compton Gamma-Rays in Galactic Medium Latitude

Zhang Li ^,

Physics Department,University of Yunnan,Kunming 650091

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Abstract：
The gamma-ray emissivity q/4π of galactic cosmic rays interacting with inter-staller gases at medium-latitude(|b|=10°—20°)is determined by using recent EGRET data. Meanwhile the method to obtain the emissivity by gamma-ray data themselve is adopted,and then the inverse compton (IC ) integral intensities as a function of galactic longitude are obtained. The differential IC intensities averaged over all galactic longitudes can be expressed by I_Ic(E)=1.58×10^－6E^{－2.08±0.06}cm^－2·s^－1·sr^－1GeV^－1,b=10°—20°and I_Ic(E)=2.08×10^－6E^{－2.03±0.06}cm^－2·s^－1·sr^－1GeV^－1,b=－20°—－10° for b=－20°—－10°,where the energy range is from 30 MeV to 4 GeV.

References

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Chi,X,et al.,J.Phys,G:15（1989）1495.[2] Chix,X.Wolfendale,A.W,J.Phys,G:17（1991）987.[3] BloemenJ.B.G M.,Astron.Astrophys,145（1985）391.[4] Fichtel C.E,Simpson G.A.,Thompson D.J,Astrophys,J.222（1978）833.[5] Osborne J,L,Wolfendale A.W,Zhang L,J.Phys,G:20（1994）1089.[6] Bertsch D.L.et al,Astroghys,J.416（1993）583.[7] Wolfendale A.W,Zhang L., J.Phys,G:20（1994）935.[8] Osborne J.L,Wolfendale A.W.,Zhang,L.,1994（inpreparation）.[9] Dame T.M,et al,Astrophys,J.322（1987）706[10] Zhang L.et al,1993,Proc.2nd Compton GRO Symposium（inpress）

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Zhang Li. Intensities of Inverse Compton Gamma-Rays in Galactic Medium Latitude[J]. Chinese Physics C, 1995, 19(11): 974-979.

Zhang Li. Intensities of Inverse Compton Gamma-Rays in Galactic Medium Latitude[J]. Chinese Physics C, 1995, 19(11): 974-979. shu

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Received: 1900-01-01
Revised: 1900-01-01

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沈阳化工大学材料科学与工程学院沈阳 110142

Intensities of Inverse Compton Gamma-Rays in Galactic Medium Latitude

Zhang Li ^,

Corresponding author: Zhang Li,

Physics Department,University of Yunnan,Kunming 650091

Received Date: 1900-01-01
Accepted Date: 1900-01-01
Available Online: 1995-11-15

Abstract: The gamma-ray emissivity q/4π of galactic cosmic rays interacting with inter-staller gases at medium-latitude(|b|=10°—20°)is determined by using recent EGRET data. Meanwhile the method to obtain the emissivity by gamma-ray data themselve is adopted,and then the inverse compton (IC ) integral intensities as a function of galactic longitude are obtained. The differential IC intensities averaged over all galactic longitudes can be expressed by I_Ic(E)=1.58×10^－6E^{－2.08±0.06}cm^－2·s^－1·sr^－1GeV^－1,b=10°—20°and I_Ic(E)=2.08×10^－6E^{－2.03±0.06}cm^－2·s^－1·sr^－1GeV^－1,b=－20°—－10° for b=－20°—－10°,where the energy range is from 30 MeV to 4 GeV.