TeV Diffuse Emission From the Inner Galaxy

被引：1
|
作者：
Nayerhoda, Amid [1 ]
Greus, Francisco Salesa [2 ]
Casanova, Sabrina [1 ]
机构：
[1] Inst Nucl Phys PAN, Krakow, Poland
[2] Max Planck Inst Nucl Phys, Heidelberg, Germany
来源：
FRONTIERS IN ASTRONOMY AND SPACE SCIENCES | 2018年 / 5卷
基金：
美国国家科学基金会;
关键词：
high energy astrophysics; inner galaxy; gamma rays; diffuse emission; cosmic rays; interstellar medium;
D O I：
10.3389/fspas.2018.00008
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The TeV diffuse emission from the Galactic plane is produced by multi TeV electrons and nuclei interacting with radiation fields and ambient gas, respectively. Measurements of the TeV diffuse emission help constrain CR origin and transport properties. We present a preliminary analysis of HAWC diffuse emission data from the inner Galaxy. The HAWC measurements will be used to constrain particle transport properties close to the Galaxy center correlating the HAWC maps with predictions of the DRAGON code.
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页数：5
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