The Nuclear X-Ray Emission-line Structure in NGC 2992 Revealed by

The Nuclear X-Ray Emission-line Structure in NGC 2992 Revealed by

We present the narrow emission-line structure revealed by a 135 ks Chandra observation of Seyfert galaxy NGC 2992, using the High Energy Transmission Grating Spectrometer. The source was observed in an historically low-flux state. Using a Bayesian Block search technique, we detected neutral Si Kα an...

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Bibliographic Details
Main Authors:	Murphy, K. D., Marshall, Herman, Nowak, Michael A.
Other Authors:	MIT Kavli Institute for Astrophysics and Space Research
Format:	Article
Published:	IOP Publishing 2017
Online Access:	http://hdl.handle.net/1721.1/112096

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