Fig. 5 from The Kinematics and Physical Conditions of the Ionized Gas in NGC 4593 from Chandra High‐Energy Grating Spectroscopy

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The Kinematics and Physical Conditions of the Ionized Gas in NGC 4593 from Chandra High‐Energy Grating Spectroscopy

Authors: Barry McKernan, Tahir Yaqoob, Ian M. George, and T. J. Turner

McKernan et al. 2003 The Astrophysical Journal 593 142.

Provider: AAS Journals

Caption: Fig. 5.

Same as Fig. 4, but showing the wavelengths of He‐like resonance‐absorption transitions (﹩n=1﹩ → 2, 3, 4, ...) of Ar, S, Si, Mg, Na, Ne, O, and N (blue) and K‐shell transitions of Fe XIX in the wavelength range 2–25 Å (red), as an illustration of some of the Fe blending in the data.

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