Cosmic ray production in Historical Supernova Remnants

被引：7
作者：
Sinitsyna, V. G. [1 ]
Sinitsyna, V. Y. [1 ]
机构：
[1] Russian Acad Sci, PN Lebedev Phys Inst, Moscow 117901, Russia
来源：
23RD EUROPEAN COSMIC RAY SYMPOSIUM (AND 32ND RUSSIAN COSMIC RAY CONFERENCE) | 2013年 / 409卷
关键词：
TEV GAMMA-RAYS; CASSIOPEIA-A; CRAB-NEBULA; GEMINGA; EMISSION; ENERGY; QUANTA; SNR; SPECTRUM; TYCHO;
D O I：
10.1088/1742-6596/409/1/012110
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We present the results of observations of two types of Galactic supernova remnants with the SHALON mirror Cherenkov telescope of Tien-Shan high-mountain Observatory: the shell-type supernova remnants Tycho, Cas A and IC 443; plerions Crab Nebula, 3c58(SN1181) and Geminga (probably plerion). The experimental data have confirmed the prediction of the theory about the hadronic generation mechanism of very high energy (800 GeV - 100 TeV) gamma-rays in Tycho's supernova remnant. The data obtained suggest that the very high energy gamma-ray emission in the objects being discussed is different in origin.
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页数：5
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