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Chandra Observations of the X-Ray Narrow-Line Region in NGC 4151

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Published 2000 November 30 © 2000. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation P. M. Ogle et al 2000 ApJ 545 L81 DOI 10.1086/317890

1538-4357/545/2/L81

Abstract

We present the first high-resolution X-ray spectrum of the Seyfert 1.5 galaxy NGC 4151. Observations with the Chandra High-Energy Transmission Grating Spectrometer reveal a spectrum dominated by narrow emission lines from a spatially resolved (1.6 kpc), highly ionized nebula. The X-ray narrow-line region is composite, consisting of both photoionized and collisionally ionized components. The X-ray emission lines have similar velocities, widths, and spatial extent to the optical emission lines, showing that they arise in the same region. The clouds in the narrow-line region must contain a large range of ionization states in order to explain both the optical and X-ray photoionized emission. Chandra data give the first direct evidence of X-ray line emission from a hot plasma (T ~ 107 K) that may provide pressure confinement for the cooler (T = 3 × 104 K) photoionized clouds.

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10.1086/317890