The ionized gas in the CALIFA early-type galaxies - I. Mapping two representative cases: NGC 6762 and NGC 5966

C. Kehrig; A. Monreal-Ibero; P. Papaderos; J. M. Vílchez; J. M. Gomes; J. Masegosa; S. F. Sánchez; M. D. Lehnert; R. Cid Fernandes; J. Bland-Hawthorn; D. J. Bomans; I. Marquez; D. Mast; J. A. L. Aguerri; Á. R. López-Sánchez; R. A. Marino; A. Pasquali; I. Perez; M. M. Roth; P. Sánchez-Blázquez; B. Ziegler

doi:10.1051/0004-6361/201118357

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Volume 540 (April 2012)

A&A, 540 (2012) A11

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Fig. 6

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Emission line ratio maps for NGC 6762 (top row) and NGC 5966 (bottom row). All maps are in logarithmic scale. The label at the top of each map indicates what emission line ratios are being displayed. The contours, linear scale, and orientation are the same as in Figs. 4 and 5.

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