Exploring the Mass Segregation Effect of X-ray Sources in Globular
  Clusters. II. The Case of Terzan 5
  Using archival {\it Chandra} observations with a total effective exposure of
734 ks, we derive an updated catalog of point sources in the massive globular
cluster Terzan 5. Our catalog covers an area of $58.1\, \rm arcmin^{2}$ ($R\leq
4.3 \, \rm arcmin$) with 489 X-ray sources, and more than $75\%$ of these
sources are first detected in this cluster. We find significant dips in the
radial distribution profiles of X-ray sources in Terzan 5, with the projected
distance and width of the distribution dips for bright ($L_{X} \gtrsim
9.5\times 10^{30} {\rm\ erg\ \,s^{-1}}$) X-ray sources are larger than that of
the faint ($L_{X} \lesssim 9.5\times 10^{30} {\rm\ erg\ \,s^{-1}}$) sources. By
fitting the radial distribution of the X-ray sources with a"generalized King
model", we estimated an average mass of $1.48\pm0.11\,M_{\odot}$ and
$1.27\pm0.13\,M_{\odot}$ for the bright and faint X-ray sources, respectively.
These results are in agreement with that observed in 47 Tuc, which may suggest
a universal mass segregation effect for X-ray sources in GCs. Compared with 47
Tuc, we show that the two-body relaxation timescale of Terzan 5 is much
smaller, but its dynamical age is significantly younger than 47 Tuc. These
features suggest that the evolution of Terzan 5 is not purely driven by
two-body relaxation, and tidal stripping effect also plays an important role in
accelerating the dynamical evolution of this cluster.
