  A Chandra observation of the non-cooling flow cluster A 1060 has confirmed
that the hot intracluster medium has fairly uniform distributions of
temperature and metal abundance from a radius of about 230 kpc to the central 5
kpc region (H_0= 75 km/s/Mpc). The radial temperature profile shows a broad
peak at 30-40 kpc from the center at a level ~20% higher than that in the outer
region. Assuming spatially uniform temperature and abundance distributions, we
derived a 3-dimensional density structure by iteratively correcting the beta
model, and obtained the central gas density to be 8.2^{+1.8}_{-1.0} x 10^{-3}
cm^{-3}. The distribution of gravitational mass was estimated from the density
profile, and a central concentration of mass within a radius of 50 kpc was
indicated. The data also suggest several high-abundance regions. The most
significant blob adjacent to the central galaxy NGC 3311 has a radius of about
9 kpc, which indicates a metallicity of ~1.5 solar. We consider that this blob
may be produced by the gas stripped off from NGC 3311.
