2014ApJ...784...79D


Query : 2014ApJ...784...79D

2014ApJ...784...79D - Astrophys. J., 784, 79 (2014/March-3)

Young star clusters in the circumnuclear region of NGC 2110.

DURRE M. and MOULD J.

Abstract (from CDS):

High-resolution observations in the near infrared show star clusters around the active galactic nucleus (AGN) of the Seyfert 1 NGC 2110, along with a 90x35 pc bar of shocked gas material around its nucleus. These are seen for the first time in our imaging and gas kinematics of the central 100 pc with the Keck OSIRIS instrument with adaptive optics. Each of these clusters is two to three times brighter than the Arches cluster close to the center of the Milky Way. The core star formation rate is 0.3 M☉/yr. The photoionized gas (He I) dynamics imply an enclosed mass of 3-4x108 M☉. These observations demonstrate the physical linkage between AGN feedback, which triggers star formation in massive clusters, and the resulting stellar (and supernovae) winds, which cause the observed [Fe II] emission and feed the black hole.

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Journal keyword(s): galaxies: active - galaxies: individual: NGC 2110 - galaxies: ISM - galaxies: nuclei - galaxies: Seyfert - galaxies: star formation

Simbad objects: 9

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Number of rows : 9
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 2110 Sy2 05 52 11.3768668776 -07 27 22.507465392   14.77 13.51 11.86   ~ 712 1
2 Cl Trumpler 14 OpC 10 43 56.0 -59 33 07   5.70 5.5     ~ 547 0
3 Cl Trumpler 16 OpC 10 45 01.9 -59 42 00           ~ 510 0
4 NGC 3372 HII 10 45 02.23 -59 41 59.8           ~ 1071 2
5 * eta Car s*b 10 45 03.545808 -59 41 03.95124 6.37 7.03 6.48 6.123 4.41 LBV 2543 0
6 NGC 4151 Sy1 12 10 32.5759813872 +39 24 21.063527532   12.18 11.48     ~ 3938 2
7 NAME Centaurus A BLL 13 25 27.61521044 -43 01 08.8050291   8.18 6.84 6.66   ~ 4774 3
8 M 13 GlC 16 41 41.634 +36 27 40.75     5.8     ~ 2291 0
9 NAME Arches Cluster Cl* 17 45 50.5 -28 49 28           ~ 792 0

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