Confirmation of nonthermal hard X-ray excess in the coma cluster from two epoch observations

被引:101
作者
Fusco-Femiano, R
Orlandini, M
Brunetti, G
Feretti, L
Giovannini, G
Grandi, P
Setti, G
机构
[1] CNR, Ist Astrofis Spaziale & Fis Cosm, I-00133 Rome, Italy
[2] CNR, IASF Bologna, I-40129 Bologna, Italy
[3] CNR, Ist Radioastron, I-40129 Bologna, Italy
[4] Univ Bologna, Dipartimento Astron, I-40127 Bologna, Italy
关键词
BL Lacertae objects : individual (1ES 1255+244); cosmic microwave background; galaxies : clusters : individual (Coma); magnetic fields; radiation mechanisms : nonthermal; X-rays : galaxies;
D O I
10.1086/382695
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We report the hard X- ray spectrum of the Coma Cluster obtained using the Phoswich Detection System data of two independent BeppoSAX observations performed with a time interval of about 3 yr. In both the spectra a nonthermal excess with respect to the thermal emission is present at a confidence level of similar to 3.4 sigma. The combined spectrum obtained by adding up the two spectra allows a measurement of the excess at the level of similar to 4.8 sigma at energies above 20 keV. The analysis of the full BeppoSAX data set provides a revised nonthermal X- ray flux that is slightly lower than that previously estimated ( Fusco- Femiano et al.) and in agreement with that measured by two Rossi X- Ray Timing Explorer observations. The analysis of the offset fields in our Coma observations provides a possible flux determination of the BL Lac object 1ES 1255 + 244.
引用
收藏
页码:L73 / L76
页数:4
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