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GLOW. I. Comprehensive Measurements of Gas-rich, Star-forming, Low-mass Galaxies in the Nearby Universe

  • Authors: Kristen B. W. McQuinn, O. Grace Telford, Roger Cohen, Liese van Zee, Laura C. Hunter, Madison Smith, Evan D. Skillman, Benjamin Williams, John M. Cannon, Joseph Burchett, Danielle A. Berg, Julianne J. Dalcanton, Andrew E. Dolphin, Suchindram Dasgupta, Avery Kiihne

Kristen B. W. McQuinn et al 2026 The Astrophysical Journal Supplement Series 287 .

  • Provider: AAS Journals

Caption: Figure 2.

LZ relation, MZ relation, and the log of the N/O abundances as a function of oxygen abundance for the GLOW sample. Points are color coded by the log of their MHI/M* ratios. Values of M* are based on the total 3.6 μm fluxes and adopting a mass-to-light ratio (see Section 4). Best-fitting lines (thicker line) and realizations within 1σ confidence intervals (thinner lines) are shown for the LZ and MZ relations.

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