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arXiv · astro-ph/9812441

ISOCAM Photometry of Narrow-Line X-ray Galaxies

J. D. Law-Green·A. Zezas·M. J. Ward·C. Boisson
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Abstract

Mid-infrared photometry of the hosts of Narrow-Line X-ray Galaxies at 6 microns and 12 microns has been attempted with ISOCAM. No conclusive detections have been made. This implies that these are quiescent objects with little or no active star-formation. Neither X-ray binaries nor starburst-driven superwinds are consistent explanations for the X-ray emission in these objects. We conclude that these NLXGs are predominantly AGN-powered.

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J. D. Law-Green, A. Zezas, M. J. Ward, C. Boisson. 1998-12-23. ISOCAM Photometry of Narrow-Line X-ray Galaxies. https://doi.org/10.1016/s0273-1177(99)00265-3

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