2001ApJ...551..730E


Query : 2001ApJ...551..730E

2001ApJ...551..730E - Astrophys. J., 551, 730-742 (2001/April-3)

Arp 220: a circumnuclear polar ring as an alternative to a double nucleus?.

ECKART A. and DOWNES D.

Abstract (from CDS):

Recent millimeter interferometer observations of Arp 220 have yielded ∼0".5 resolution images showing two strong concentrations of millimeter radio continuum and CO line emission embedded in a larger molecular gas disk (r∼1 kpc). The interferometer observations also revealed a complex velocity field with steep velocity gradients across each of the flux concentrations of Δv∼500 km.s–1 within r=0".3. The directions of these gradients are not aligned with each other or with that of the outer gas disk. This led to the conclusion that the two emission peaks represent either double nuclei with their own gas disks (r∼100 pc), which are counterrotating with respect to each other and rotate around the dynamical center of the system, or that they are two hot spots within a nuclear molecular gas disk. The overall structure of the molecular gas distribution and the corresponding complex velocity field, however, are highly symmetric, except for the unequal brightnesses of the two flux concentrations. This fact and similarities to the distribution and kinematics of the molecular gas in the central 2'' of NGC 1068 motivated us to try describing the Arp 220 nucleus as a warped molecular gas disk in which the peaks in the flux and line width distributions arise as a result of crowding of inclined circular orbits. Hubble Space Telescope (HST) images of the dust lanes flaring toward larger radii provide further support for a warped gas disk. The final model is surprisingly successful in explaining the CO line flux distribution, the velocity field, and position-velocity diagrams across the central flux concentrations. The model represents a strong 90° warp of the gas orbits out of the principal plane forming a circumnuclear polar ring and reproduces well the structures in HST near-IR color and continuum maps. The large number of young stars recently formed out of the warped, polar-ring gas implies that those stars will have kinematic properties similar to that of the molecular gas. We suggest that the red near-IR source at the center of the polar ring is the true nucleus of Arp 220. The success of the model implies that the two flux concentrations are not necessarily counterrotating nuclei, but rather the result of a combination of hot spots and orbit crowding due to the warp. The warp could be a direct consequence of the recent merger event indicated by tidal tails in optical images.

Abstract Copyright: ∼

Journal keyword(s): galaxies: individual (Arp 220) - Galaxies: ISM - Galaxies: Kinematics and Dynamics - Galaxies: Nuclei - Radio Lines: Galaxies

Simbad objects: 12

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Number of rows : 12
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 NGC 128 GiG 00 29 15.0429950112 +02 51 50.564329164   13.2       ~ 210 0
2 NGC 253 SyG 00 47 33.134 -25 17 19.68   8.03   6.94 8.1 ~ 3588 2
3 IC 1689 GiG 01 23 47.8730638824 +33 03 19.075686660   14.8       ~ 55 0
4 NGC 524 GiP 01 24 47.7429545736 +09 32 20.089023900   11.5       ~ 494 1
5 M 77 Sy2 02 42 40.7091669408 -00 00 47.859690204 9.70 9.61 8.87 10.1 9.9 ~ 4897 2
6 NGC 2685 Sy2 08 55 34.7027817000 +58 44 03.876540108   13.68 12.70     ~ 459 1
7 NGC 2841 LIN 09 22 02.6778711696 +50 58 35.737082868 10.43 10.09 9.22     ~ 1113 1
8 NGC 3227 Sy1 10 23 30.5765149296 +19 51 54.282206700   12.61 11.79     ~ 1807 2
9 IC 1127 SyG 15 34 57.22396 +23 30 11.6084   14.76 13.88     ~ 3090 4
10 NGC 6340 GiP 17 10 24.8346254376 +72 18 15.919996608   11.87 11.01     ~ 197 1
11 NGC 7217 LIN 22 07 52.3984675584 +31 21 33.632293572   12.94 11.92     ~ 511 0
12 [BH95] C Rad ~ ~           ~ 5 0

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