Figure 2 from Characterizing the Circumgalactic Medium of Nearby Galaxies with HST/COS and HST/STIS Absorption-line Spectroscopy. II. Methods and Models

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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 2.

Comparison of the stellar mass (﹩{M}_{* }﹩) and specific star-formation rate (sSFR) of the targeted and serendipitous galaxies with those of the COS-Halos and COS-Dwarfs samples. Our sample includes several galaxies (both targeted and serendipitous) that are less massive than any COS-Dwarfs galaxy.

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