Fig. 3 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. 3.

Confidence contours for the line energy and intensity. The energy scale is redshift corrected. The contours correspond to 68%, 90%, and 99% confidence level for two interesting parameters (Δχ² = 2.3, 4.6, and 9.2, respectively).

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