The Central Region of the Nearby Seyfert 2 Galaxy NGC 4945: A Pair of Spirals
Artikel i vetenskaplig tidskrift, 2011

NGC 4945 is a Seyfert 2 galaxy at a distance of 3.82 Mpc. Its relative proximity has permitted a detailed Submillimeter Array study of the circumnuclear molecular gas in a galaxy exhibiting an active galactic nucleus (AGN). Based on an analysis of the high-resolution velocity field of the central region (20 '' x 20 '', 1 '' = 19 pc), we demonstrate that the S-shaped structure of the isovelocity contours is well reproduced by the numerical results of a two-dimensional hydrodynamical simulation. In particular, the velocity structure is represented by the bending produced by a shock along the spiral density waves, which are excited at the outer-inner Lindblad resonance (OILR) by a fast rotating bar. The simulated density map reveals a pair of tightly wound spirals in the center which pass through most of the ring-like (claimed to be a circumnuclear starburst ring by other authors) high-intensity region in the observations as well as intersect several Paa emission line knots located outside the ring-like region. The calculated mass inflow rate at a scale of 50 pc is about three times the inferred mass accretion rate of the AGNs of NGC 4945. We find that self-gravity of the gas is important and should be included in our model for NGC 4945. The model is compared with the gas orbit model discussed in Lim et al., and it is shown that the hydrodynamic model provides a better match to the observed position-velocity diagram and, hence, provides a more reliable prediction of the OILR position.

disks

galaxies: spiral

galaxies: kinematics and dynamics

galaxies: structure

hydrodynamical simulations

dynamical interpretation

galaxies: individual (NGC 4945)

nuclear spirals

ngc-4945

gas response

barred galaxies

diagnostics

kinematics

gasdynamics

Författare

L. H. Lin

Institute of Astrophysics and Astronomy, Academia Sinica Taiwan

R. E. Taam

Institute of Astrophysics and Astronomy, Academia Sinica Taiwan

Northwestern University

D. C. C. Yen

Fu Jen Catholic University

Sebastien Muller

Chalmers, Rymd- och geovetenskap, Onsala rymdobservatorium

J. Lim

The University of Hong Kong

Institute of Astrophysics and Astronomy, Academia Sinica Taiwan

Astrophysical Journal

0004-637X (ISSN) 1538-4357 (eISSN)

Vol. 731 15

Ämneskategorier

Astronomi, astrofysik och kosmologi

DOI

10.1088/0004-637x/731/1/15