Significant X-ray Line Emission in the 5-6 keV band of NGC 4051
A Suzaku X-ray observation of NGC 4051 taken during 2005 Nov reveals line emission at 5.44 keV in the rest-frame of the galaxy which does not have an obvious origin in known rest-frame atomic transitions. The improvement to the fit statistic when this line is accounted for establishes its reality at...
Main Authors: | Turner, T, Miller, L, Reeves, J, Lobban, A, Braito, V, Kraemer, S, Crenshaw, D |
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格式: | Journal article |
语言: | English |
出版: |
Institute of Physics Publishing
2010
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