Evidence for azimuthal variations of the oxygen abundance gradient
tracing the spiral structure of the galaxy HCG91c
F. Vogt, E. Pérez, M. Dopita, L. Verdes-Montenegro, and S. Borthakur. (2017)cite arxiv:1701.01728Comment: 12 pages, 11 figures, accepted for publication in A&A. Supplementary movie assocociated with Fig. 8 is available (until publication) at: http://www.sc.eso.org/~fvogt/supp_mat/HCG91c/O_gradient.mp4.
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