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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. 13.

Curves of growth for various values of the velocity width, b. Plotted for each b‐value is the logarithm of line equivalent width (EW) per unit wavelength against the logarithm of the product of ionic column density (N), oscillator strength (f), and wavelength (λ). The plotted points are taken from the measured equivalent widths (converted to angstroms by using the values in Table 1) and predicted ionic column densities (from the best‐fitting XSTAR model described in § 5). These values are consistent with ﹩b=200﹩ km s−1 within errors.

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