The unusual morphology of the intragroup medium in NGC 5171

Details The unusual morphology of the intragroup medium in NGC 5171 The unusual morphology of the intragroup medium in NGC 5171

2004-08-11

arxiv.org/abs/astro-ph/0408206v1

Astronomy and Astrophysics

Astrophysics

10 pages, 8 figures, to be published in MNRAS

Scientific paper

10.1111/j.1365-2966.2004.08298.x

We present the results of a 24 ks XMM-Newton observation of the NGC 5171 group of galaxies. NGC 5171 is unusual in that it is an X-ray bright group (L > 10^42 erg/s), with irregular contours which are not centred on a bright galaxy. The global spectrum is adequately described by a single temperature APEC model with T = 0.96 +/- 0.04 keV, and Z = 0.13 +/- 0.02 Zsol, in good agreement with previous ROSAT data. We find the X-ray contours are centred on a bright ridge of emission stretching from the BGG to a nearby galaxy. Spectral mapping reveals this ridge to be both cool (T ~ 1.1 keV) and metallic (Z ~ 0.4 Zsol) in comparison to its surrounding, suggesting it is the result of a tidal interaction between the two galaxies. Optical data reveals the member galaxies to have a high velocity dispersion (sigma = 494 +/- 99 km/s), and a significantly non-Gaussian velocity distribution, suggesting the group is in the process of merging. A region of hot gas with T = 1.58 +/- 0.36 keV is found to the West of the bright central ridge, and we interpret this as shock-heating resulting from the merging. A further region of emission to the South-East of the bright central ridge, with T = 1.14 +/- 0.13 keV, is probably associated with a background group, four times more distant.

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