Hard X-ray emission from Cassiopeia A SNR

被引:0
|
作者
The, LS [1 ]
Leising, MD [1 ]
Hartmann, DH [1 ]
Kurfess, JD [1 ]
Blanco, P [1 ]
Bhattacharya, D [1 ]
机构
[1] Clemson Univ, Dept Phys & Astron, Clemson, SC 29634 USA
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P1 [天文学];
学科分类号
0704 ;
摘要
We report the results of extracting the hard X-ray continuum spectrum of Cas A SNR from RXTE/PCA Target of Opportunity (TOO) observations and CGRO/OSSE observations. The data can rule out the single thermal bremsstrahlung model for Cas A continuum between 2 and 150 keV. The single power law model gives a mediocre fit (similar to 5%) to the data with a power-law index, Gamma = 2.94+/-0.02. A model with two component (bremsstrahlung + bremsstrahlung or bremsstrahlung + power law) gives a good fit. The power law index is quite constrained suggesting that this continuum might not be tbe X-ray thermal bremmstrahlung from accelerated MeV electrons at shock fronts [1] which would have Gamma similar or equal to 2.26. With several SNRs detected by ASCA showing a hard power-law nonthermal X-ray continuum, we expect a similar situation for Cas A SNR which has Gamma=2.98+/-0.09. We discuss the implication of the hardest nonthermal X-rays detected from Cas A to the synchrotron radiation model.
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页码:1147 / 1151
页数:5
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