2011ApJ...741...38G


Query : 2011ApJ...741...38G

2011ApJ...741...38G - Astrophys. J., 741, 38 (2011/November-1)

Is there a black hole in NGC 4382?

GULTEKIN K., RICHSTONE D.O., GEBHARDT K., FABER S.M., LAUER T.R., BENDER R., KORMENDY J. and PINKNEY J.

Abstract (from CDS):

We present Hubble Space Telescope (HST) Space Telescope Imaging Spectrograph observations of the galaxy NGC 4382 (M85) and axisymmetric models of the galaxy to determine mass-to-light ratio (ΥV) and central black hole mass (MBH). We find ΥV= 3.74±0.1 M{x2609}/L{x2609} and MBH= 1.3+5.2_- 1.2_x107 M{x2609}at an assumed distance of 17.9 Mpc, consistent with no black hole. The upper limit, MBH< 9.6 x107 M{x2609}(2σ) or MBH< 1.4x108(3σ), is consistent with the current M-σ relation, which predicts MBH= 8.8x107 M{x2609} at σe= 182 km/s, but low for the current M - L relation, which predicts MBH= 7.8x108 M{x2609} at LV= 8.9 x1010 L_{x2609}, V_. HST images show the nucleus to be double, suggesting the presence of a nuclear eccentric stellar disk, analogous to the Tremaine disk in M31. This conclusion is supported by the HST velocity dispersion profile. Despite the presence of this non-axisymmetric feature and evidence of a recent merger, we conclude that the reliability of our black hole mass determination is not hindered. The inferred low black hole mass may explain the lack of nuclear activity.

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Journal keyword(s): black hole physics - galaxies: individual (NGC 4382, M85) - galaxies: kinematics and dynamics - galaxies: nuclei

Simbad objects: 5

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Number of rows : 5
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 M 31 AGN 00 42 44.330 +41 16 07.50 4.86 4.36 3.44     ~ 13622 1
2 NGC 3945 GiG 11 53 13.6081388304 +60 40 32.125024704   11.6       ~ 265 0
3 M 85 GiP 12 25 24.053 +18 11 27.89   10.2       ~ 678 0
4 NGC 4395 Sy2 12 25 48.8633109888 +33 32 48.700168152 10.84 10.54 10.11 9.98   ~ 1286 1
5 M 87 AGN 12 30 49.42338414 +12 23 28.0436859 10.16 9.59 8.63   7.49 ~ 7815 3

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