Fig. 3 from An ASCA Observation of M51 (NGC 5194): Iron K Emission from an Obscured Active Galactic Nucleus

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An ASCA Observation of M51 (NGC 5194): Iron K Emission from an Obscured Active Galactic Nucleus

Authors: Y. Terashima, A. Ptak, R. Fujimoto, M. Itoh, H. Kunieda, K. Makishima, and P. J. Serlemitsos

Terashima et al. 1998 The Astrophysical Journal 496 210.

Provider: AAS Journals

Caption: Fig. 3.

ASCA SIS and GIS spectra of M51. The solid lines represent the best‐fit model of a combination of a variable‐abundance Raymond‐Smith model, a power law, and a Gaussian.

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