Very high energy gamma rays from the composite SNR G0.9+0.1

被引:166
作者
Aharonian, F
Akhperjanian, AG
Aye, KM
Bazer-Bachi, AR
Beilicke, M
Benbow, W
Berge, D
Berghaus, P
Bernlöhr, K
Boisson, C
Bolz, O
Borgmeier, C
Braun, I
Breitling, F
Brown, AM
Gordo, JB
Chadwick, PM
Chounet, LM
Cornils, R
Costamante, L
Degrange, B
Djannati-Ataï, A
Drury, LO
Dubus, G
Ergin, T
Espigat, P
Feinstein, F
Fleury, P
Fontaine, G
Funk, S
Gallant, YA
Giebels, B
Gillessen, S
Goret, P
Hadjichristidis, C
Hauser, M
Heinzelmann, G
Henri, G
Hermann, G
Hinton, JA
Hofmann, W
Holleran, M
Horns, D
de Jager, OC
Jung, I
Khélifi, B
Komin, N
Konopelko, A
Latham, IJ
Le Gallou, R
机构
[1] Max Planck Inst Kernphys, D-69029 Heidelberg, Germany
[2] Yerevan Phys Inst, Yerevan 375036, Armenia
[3] Univ Durham, Dept Phys, Durham DH1 3LE, England
[4] UPS, CNRS, Ctr Etud Spatiale Rayonnements, F-31029 Toulouse 4, France
[5] Univ Hamburg, Inst Expt Phys, D-22761 Hamburg, Germany
[6] Coll France, CNRS, IN2P3, F-75231 Paris 05, France
[7] Humboldt Univ, Inst Phys, D-12489 Berlin, Germany
[8] Observ Paris, Sect Meudon, LUTH, CNRS,UMR 8102, F-92195 Meudon, France
[9] Univ Montpellier 2, Grp Astroparticules Montpellier, CNRS, IN2P3, F-34095 Montpellier 5, France
[10] Ecole Polytech, Lab Leprince Ringuet, CNRS, IN2P3, F-91128 Palaiseau, France
[11] Dublin Inst Adv Studies, Dublin 2, Ireland
[12] Ctr Etud Saclay, CEA, DSM, DAPNIA,Serv Astrophys, F-91191 Gif Sur Yvette, France
[13] Landessternwarte Konigstuhl, D-69117 Heidelberg, Germany
[14] Univ Grenoble 1, Lab Astrophys Grenoble, CNRS, INSU, F-38041 Grenoble 9, France
[15] North West Univ, Unit Space Phys, ZA-2520 Potchefstroom, South Africa
[16] Univ Paris 06, Lab Phys Nucl & Hautes Energies, CNRS, IN2P3, F-75231 Paris 05, France
[17] Ruhr Univ Bochum, Inst Theoret Phys, Lehrstuhl Weltraum & Astrophys 4, D-44780 Bochum, Germany
[18] Charles Univ, Inst Nucl & Particle Phys, CR-18000 Prague 8, Czech Republic
[19] Univ Namibia, Windhoek, Namibia
来源
ASTRONOMY & ASTROPHYSICS | 2005年 / 432卷 / 02期
关键词
ISM : supernova remnants; ISM : individual objects : G0.9+0.1; gamma-rays : observations;
D O I
10.1051/0004-6361:200500022
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Very high energy (> 100 GeV) gamma-ray emission has been detected for the first time from the composite supernova remnant G0.9+ 0.1 using the HESS instrument. The source is detected with a significance of approximate to 13sigma, and a photon flux above 200 GeV of ( 5.7 +/- 0.7(stat) +/- 1.2(sys)) x 10(-12) cm(-2) s(-1), making it one of the weakest sources ever detected at TeV energies. The photon spectrum is compatible with a power law ( dN/dE proportional to E-Gamma) with photon index Gamma = 2.40 +/- 0.11(stat) +/- 0.20(sys). The gamma-ray emission appears to originate in the plerionic core of the remnant, rather than the shell, and can be plausibly explained as inverse Compton scattering of relativistic electrons.
引用
收藏
页码:L25 / L29
页数:5
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