Significant X-ray Line Emission in the 5-6 keV band of NGC 4051

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...

書誌詳細
主要な著者:	Turner, T, Miller, L, Reeves, J, Lobban, A, Braito, V, Kraemer, S, Crenshaw, D
フォーマット:	Journal article
言語:	English
出版事項:	Institute of Physics Publishing 2010

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