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.

引用

页码：304 / +

页数：3

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