Fig. 1 from Detection of an Iron K Emission Line from the LINER NGC 4579

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Detection of an Iron K Emission Line from the LINER NGC 4579

Authors: Yuichi Terashima, Hideyo Kunieda, Kazutami Misaki, Richard F. Mushotzky, Andrew F. Ptak, and Gail A. Reichert

Terashima et al. 1998 The Astrophysical Journal 503 212.

Provider: AAS Journals

Caption: Fig. 1.

ASCA (a) SIS and (b) GIS spectra of NGC 4579. The best‐fit model consists of an R‐S thermal plasma, a power law, and a Gaussian and is shown as histograms. SIS and GIS data are plotted separately for clarity.

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