Figure 7 from A KECK ADAPTIVE OPTICS SURVEY OF A REPRESENTATIVE SAMPLE OF GRAVITATIONALLY LENSED STAR-FORMING GALAXIES: HIGH SPATIAL RESOLUTION STUDIES OF KINEMATICS AND METALLICITY GRADIENTS

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A KECK ADAPTIVE OPTICS SURVEY OF A REPRESENTATIVE SAMPLE OF GRAVITATIONALLY LENSED STAR-FORMING GALAXIES: HIGH SPATIAL RESOLUTION STUDIES OF KINEMATICS AND METALLICITY GRADIENTS

Authors: Nicha Leethochawalit, Tucker A. Jones, Richard S. Ellis, Daniel P. Stark, Johan Richard, Adi Zitrin, and Matthew Auger

2016 The Astrophysical Journal 820 84.

Provider: AAS Journals

Caption: Figure 7.

Correlation between the observed metallicity gradient for the present sample (L15) (Jones et al. 2013, J13 and Swinbank et al. 2012, S12) and the integrated [N II]/Hα ratio (left panel) and the star formation rate (right panel). Filled symbols represent isolated galaxies; open symbols represent interacting and/or kinematically immature galaxies.

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