2008A&A...482..133H


C.D.S. - SIMBAD4 rel 1.7 - 2020.07.02CEST14:16:54

2008A&A...482..133H - Astronomy and Astrophysics, volume 482, 133-150 (2008/4-4)

Molecular Gas in NUclei of GAlaxies (NUGA). IX. The decoupled bars and gas inflow in NGC2782.

HUNT L.K., COMBES F., GARCIA-BURILLO S., SCHINNERER E., KRIPS M., BAKER A.J., BOONE F., ECKART A., LEON S., NERI R. and TACCONI L.J.

Abstract (from CDS):

We present CO(1-0) and CO(2-1) maps of the starburst/Seyfert1 galaxy NGC2782 obtained with the IRAM interferometer, at 2.1"x1.5" and 0.7"x0.6" resolution respectively. The CO emission is aligned along the stellar nuclear bar of radius ∼1kpc, configured in an elongated structure with two spiral arms at high pitch angle ∼90°. At the extremity of the nuclear bar, the CO changes direction to trace two more extended spiral features at a lower pitch angle. These are the beginning of two straight dust lanes, which are aligned parallel to an oval distortion, reminiscent of a primary bar, almost perpendicular to the nuclear one. The two embedded bars appear in Spitzer IRAC near-infrared images, and HST color images, although highly obscured by dust in the latter. We compute the torques exerted by the stellar bars on the gas, and find systematically negative average torques down to the resolution limit of the images, providing evidence of gas inflow tantalizingly close to the nucleus of NGC2782. We propose a dynamical scenario based on numerical simulations to interpret coherently the radio, optical, and molecular gas features in the center of the galaxy. Star formation is occurring in a partial ring at ∼1.3kpc radius corresponding to the Inner Lindblad Resonance (ILR) of the primary bar; this ring-like structure encircles the nuclear bar, and is studded with Hα emission. The gas traced by CO emission is driven inward by the gravity torques of the decoupled nuclear bar, since most of it is inside its corotation. N-body simulations, including gas dissipation, predict the secondary bar decoupling, the formation of the elongated ring at the ∼1kpc-radius ILR of the primary bar, and the gas inflow to the ILR of the nuclear bar at a radius of ∼200-300pc. The presence of molecular gas inside the ILR of the primary bar, transported by a second nuclear bar, is a potential ``smoking gun''; the gas there is certainly fueling the central starburst, and in a second step could fuel directly the AGN.

Abstract Copyright:

Journal keyword(s): galaxies: individual: NGC 2782 - galaxies: starburst - galaxies: spiral - galaxies: kinematics and dynamics - galaxies: ISM

Simbad objects: 13

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Number of rows : 13

N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2020
#notes
1 NGC 2782 Sy2 09 14 05.120 +40 06 49.68 12.29 12.30 11.63     ~ 431 3
2 ICRF J092703.0+390220 Sy1 09 27 03.0139516273 +39 02 20.847968628   17.17 17.00 16.486   ~ 932 1
3 NGC 2997 GiG 09 45 38.7537949543 -31 11 27.357027761   9.97 9.41 8.84 9.9 ~ 378 0
4 M 82 IG 09 55 52.430 +69 40 46.93 9.61 9.30 8.41     ~ 5331 6
5 NGC 3718 GiP 11 32 34.8527469396 +53 04 04.494313634   11.35 10.61     ~ 342 1
6 NGC 4314 LIN 12 22 31.978 +29 53 43.09 11.72 11.43 10.58     ~ 449 1
7 M 100 AGN 12 22 54.9318850854 +15 49 20.294302163 10.04 10.05 9.35     ~ 1646 2
8 3C 273 BLL 12 29 06.6996828061 +02 03 08.598846466   13.05 14.830 14.11   ~ 5313 1
9 M 90 Sy2 12 36 49.816 +13 09 46.33 10.56 10.26 9.54     ~ 794 1
10 M 58 SyG 12 37 43.597 +11 49 05.12 10.80 10.48 9.66     ~ 968 2
11 M 64 SyG 12 56 43.696 +21 40 57.57   9.36 8.52     ~ 812 2
12 NGC 6951 Sy2 20 37 14.1181441937 +66 06 20.078027288   11.64 10.65     ~ 497 2
13 NGC 7217 LIN 22 07 52.368 +31 21 33.32   12.94 11.92     ~ 461 0

    Equat.    Gal    SGal    Ecl

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2020.07.02-14:16:54

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