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. 12

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Kinematics maps of NGC 6762 (top row) and NGC 5966 (bottom row): stellar velocity field (left panels), corrected velocity dispersion maps (middle panels) and radial velocity maps (right panels), as measured from Hα. The contours, orientation, and linear scale are the same as in Figs. 4 and 5.

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