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What is NGC 4151 X-ray Emission Study about?

This document summarizes a study using Chandra observations of the Seyfert galaxy NGC 4151. The observations allow high spatial resolution imaging of emission lines like OVII, OVIII, and NeIX within 150 pc of the galaxy center. The maps show extensions spatially correlated with the radio outflow and optical emission, providing evidence for interaction between the radio jet and gas clouds. The observations also place constraints on the spatial origin of iron Kα emission in the galaxy, disagreeing with a prio

Author

Sayee Chandrasekaramouli

Language

EN