Chandra Observation of the Cluster of Galaxies MS 0839.9+2938 at z=0.194 the Central Excess.pdf
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Chandra Observation of the Cluster of Galaxies MS 0839.9+2938
at z = 0.194: the Central Excess Iron and SN Ia Enrichment
Yu Wang1,2,3, Haiguang Xu1, Zhongli Zhang1, Yueheng Xu1, Xiang-Ping Wu2, Sui-Jian
Xue2, and Zongwei Li3
ABSTRACT
We present the Chandra study of the intermediately distant (z = 0.194)
cluster of galaxies MS 0839.9+2938. By performing both the projected and
deprojected spectral analyses, we find that the gas temperature is approximately
constant at about 4 keV in 130 ? 444h?170 kpc. In the inner regions, the gas
temperature descends towards the center, reaching
~
3 keV in the central 37h?170
kpc. This infers that the lower and upper limits of the mass deposit rate are
9?34M⊙ yr?1 and 96?126M⊙ yr?1, respectively within 74h?170 kpc where the gas
is significantly colder. Along with the temperature drop, we detect a significant
inward iron abundance increase from about 0.4 solar in the outer regions to ?1
solar within the central 37h?170 kpc. Thus MS 0839.9+2938 is the cluster showing
the most significant central iron excess at z
~
0.2. We argue that most of the
excess iron should have been contributed by SNe Ia. By utilizing the observed
SN Ia rate and stellar mass loss rate, we estimate that the time needed to enrich
the central region with excess iron is 6.4 ? 7.9 Gyr, which is similar to those
found for the nearby clusters. Coinciding with the optical extension of the cD
galaxy (up to about 30h?170 kpc), the observed X-ray surface brightness profile
exhibits an excess beyond the distribution expected by either the β model or the
NFW model, and can be well fitted with an empirical two-β model that leads to
a relatively flatter mass profile in the innermost region.
Subject headings: galaxies: clusters: individual (MS 0839.9+2938) — intergalac-
tic medium — galaxies: evolution — X-rays: galaxies: clusters
1Department of Physics, Shanghai Jiao Tong University, 1954 Huashan Road, Sh
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