Discovery of SN 1006 in VHE Gamma-Rays by HESS

被引：0
|
作者：
Godo, M. Naumann [1 ]
Beilicke, A. [2 ]
Hauser, D. [3 ,4 ]
Goumard, M. Lemoine [5 ]
de Naurois, M. [6 ]
机构：
[1] Ecole Polytech, CNRS, IN2P3, Lab Leprince Ringuet, F-91128 Palaiseau, France
[2] Washington Univ, Dept Phys, St Louis, MO 63130 USA
[3] Max Planck Inst Kernphys, D-69029 Heidelberg, Germany
[4] Landessternwarte Heidelberg, D-69117 Heidelberg, Germany
[5] CEN Bordeaux Gradignan, F-33175 Gradignan, France
[6] Univ Paris 06 & 07, IN2P3, CNRS, Lab Phys Nucl Hautes Energies, F-75231 Paris, France
来源：
HIGH ENERGY GAMMA-RAY ASTRONOMY | 2009年 / 1085卷
基金：
英国科学技术设施理事会; 新加坡国家研究基金会;
关键词：
Gamma rays; supernova remnants; SN; 1006; morphology; SN-1006; EMISSION; REMNANT;
D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Recent theoretical predictions of the TeV-luminosity of SN 1006 under various scenarii are only a factor of 2 to 3 below the previously published H.E.S.S. upper limit, thus motivating further in-depth observations of this source. After analysing more than 100 hours of accumulated H.E.S.S. data a signal associated with the remnant of SN 1006 has finally been detected. The measured gamma-ray flux is of order 1% that detected from the Crab Nebula, consistent with the previously established H.E.S.S. upper limit. The new results and morphological comparisons with X-ray data on this source is presented at the conference.
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页码：304 / +
页数：3
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