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Characterizing the Circumgalactic Medium of Nearby Galaxies with HST/COS and HST/STIS Absorption-line Spectroscopy. II. Methods and Models

  • Authors: Brian A. Keeney, John T. Stocke, Charles W. Danforth, J. Michael Shull, Cameron T. Pratt, Cynthia S. Froning, James C. Green, Steven V. Penton, and Blair D. Savage

2017 The Astrophysical Journal Supplement Series 230 6.

  • Provider: AAS Journals

Caption: Figure 10.

Distribution of H I column density for absorbers with and without metals (top) and with and without O VI absorption specifically (bottom). In the top panel no constraints are placed on the strength of the metal-line absorption or lack thereof. In the bottom panel, a cutoff of ﹩{N}_{{\rm{O}}{\rm{VI}}}={10}^{13.2}\,{\mathrm{cm}}^{-2}﹩ is used for the presence or absence of O VI absorption (i.e., only O VI absorbers with larger column densities are considered, and O VI must be detectable at the cutoff column density to at least ﹩3\sigma ﹩ significance for O VI nondetections).

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