The Astrophysical Journal, 806:84 (22pp), 2015 June 10 doi:10.1088/0004-637X/806/1/84 © 2015. The American Astronomical Society. All rights reserved. THE COMPLEX GAS KINEMATICS IN THE NUCLEUS OF THE SEYFERT 2 GALAXY NGC 1386: ROTATION, OUTFLOWS, AND INFLOWS D. Lena1, A. Robinson1, T. Storchi-Bergman2,7, A. Schnorr-Müller3,4, T. Seelig1, R. A. Riffel5, N. M. Nagar6, G. S. Couto2, and L. Shadler1 1 School of Physics and Astronomy, Rochester Institute of Technology, 84 Lomb Memorial Drive, Rochester, NY 14623-5603, USA;
[email protected] 2 Instituto de Fisica, Universidade Federal do Rio Grande do Sul, 91501-970, Porto Alegre, Brazil 3 Max-Planck-Institut für extraterrestrische Physik, Giessenbachstr. 1, D-85741, Garching, Germany 4 CAPES Foundation, Ministry of Education of Brazil, 70040-020, Braslia, Brazil 5 Universidade Federal de Santa Maria, Departamento de Fisica, 97105-900, Santa Maria, RS, Brazil 6 Astronomy Department, Universidad de Concepción, Casilla 160-C, Concepción, Chile 7 Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA Received 2014 October 3; accepted 2015 April 19; published 2015 June 9 ABSTRACT We present optical integral field spectroscopy of the circum-nuclear gas of the Seyfert 2 galaxy NGC 1386. The data cover the central 7″ ×9″ (530 × 680 pc) at a spatial resolution of 0″.9 (68 pc), and the spectral range − 5700–7000 Å at a resolution of 66 km s 1. The line emission is dominated by a bright central component, with two lobes extending ≈3″ north and south of the nucleus. We identify three main kinematic components.