2004MNRAS.349.1240K


Query : 2004MNRAS.349.1240K

2004MNRAS.349.1240K - Mon. Not. R. Astron. Soc., 349, 1240-1250 (2004/April-3)

An old galaxy group: Chandra X-ray observations of the nearby fossil group NGC 6482.

KHOSROSHAHI H.G., JONES L.R. and PONMAN T.J.

Abstract (from CDS):

We present the first detailed X-ray observations, using Chandra, of NGC 6482 - the nearest known fossil group. The group is dominated by an optically luminous giant elliptical galaxy and all other known group members are at least two magnitudes fainter. The global X-ray properties (luminosity, temperature, extent) of NGC 6482 fall within the range of other groups, but the detailed properties show interesting differences. We derive the gas temperature and total mass profiles for the central 30 h –170kpc (∼0.1 r200) using ACIS spatially resolved spectroscopy. The unusually high LX/Loptratio is found to result from a high central gas density. The temperature profile shows a continuous decrease outward, dropping to 0.63 of its central value at 0.1r200. The derived total mass profile is strongly centrally peaked, suggesting an early formation epoch. These results support a picture in which fossil groups are old, giving time for the most massive galaxies to have merged (via the effects of dynamical friction) to produce a central giant elliptical galaxy.

Although the cooling time within 0.1r200is less than a Hubble time, no decrease in central temperature is detected. The entropy of the system lies toward the low side of the distribution seen in poor groups and drops all the way into the centre of the system, reaching very low values. No isentropic core, such as those predicted in simple pre-heating models, is present. Given the lack of any central temperature drop in the system, it seems unlikely that radiative cooling can be invoked to explain this low central entropy. The lack of any signature of central cooling is especially striking in a system that appears to be old and relaxed, and to have a central cooling time ≤108 yr. We find that the centrally peaked temperature profile is consistent with a steady-state cooling-flow solution with an accretion rate of 2 M☉/yr, given the large P dV work arising from the cuspy mass profile. However, solutions involving distributed or non-steady heating cannot be ruled out.


Abstract Copyright: 2004 RAS

Journal keyword(s): galaxies: clusters: general - galaxies: elliptical and lenticular, cD - galaxies: haloes - intergalactic medium - X-rays: galaxies - X-rays: galaxies: clusters

Simbad objects: 11

goto Full paper

goto View the references in ADS

Number of rows : 11
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 1550 BiC 04 19 37.9450450152 +02 24 35.918168940   14.0       ~ 183 1
2 NGC 2563 GiG 08 20 35.6870161656 +21 04 04.111020012   13.7 12.39     ~ 163 1
3 ACO 1413 ClG 11 55 12.87 +23 23 46.9           ~ 456 0
4 NGC 4325 BiC 12 23 06.662 +10 37 16.45   15.0       ~ 140 1
5 ACO 1983 ClG 14 52 59.33 +16 46 11.0           ~ 249 1
6 Z 141-14 GiG 17 50 21.22 +22 57 04.6   15.5       ~ 8 0
7 Z 141-15 GiG 17 50 45.7734061632 +23 08 19.040808696   15.3       ~ 22 0
8 NAME NGC 6482 Group ClG 17 51 47.5 +23 04 14           ~ 20 0
9 NGC 6482 GiG 17 51 48.8339247888 +23 04 18.889271112 12.71 12.35 11.45     ~ 220 1
10 UGC 11018 AG? 17 52 22.38 +22 52 19.5   17       ~ 10 0
11 Z 141-24 GiG 17 52 54.5107015272 +23 12 40.029461172   15.0       ~ 28 0

To bookmark this query, right click on this link: simbad:objects in 2004MNRAS.349.1240K and select 'bookmark this link' or equivalent in the popup menu