Astronomy and Astrophysics – Astrophysics
Scientific paper
1999-06-25
Mon.Not.Roy.Astron.Soc. 307 (1999) 722-724
Astronomy and Astrophysics
Astrophysics
3 pages, to appear in MNRAS
Scientific paper
10.1046/j.1365-8711.1999.02677.x
Redshifts of several galaxies thought to be associated with NGC 326 are determined. The results confirm the presence of a cluster and find a mean redshift of z = 0.0477 +/- 0.0007 and a line-of-sight velocity dispersion sigma_{z} = 599 (+230, -110) km/s. The velocity dispersion and previously measured X-ray gas temperature of kT ~ 1.9 keV are consistent with the cluster sigma_{z}/kT relation, and NGC 326 is seen to be a slowly-moving member of the cluster.
Birkinshaw Mark
Werner P. N.
Worrall Diana Mary
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