  We present a multiwavelength investigation of the hub-filament system RCW 117
(IRAS 17059-4132), which shows intricate filamentary features in the
far-infrared, mapped using Herschel images. We obtain the column density and
dust temperature maps for the region using the Herschel images, and identify 88
cores and 12 filaments from the column density map of the region
($18'\times18'$). We employ the ThrUMMS $^{13}$CO (J=1-0) data for probing the
kinematics in RCW 117, and find velocity gradients ($\sim 0.3-1$ km s$^{-1}$
pc$^{-1}$) with hints of matter inflow along the filamentary structures.
Ionised gas emission from the associated HII region is examined using the Giant
Metrewave Radio Telescope (GMRT) at 610 and 1280 MHz, and is found to be of
extent $5 \times 3$ pc$^2$ with intensity being brightest towards the hub. We
estimate the peak electron density towards the hub to be $\sim 750$ cm$^{-3}$.
Thirty four Class 0/I young stellar objects (YSOs) have been identified in the
region using the Spitzer GLIMPSE colour-colour diagram, with many lying along
the filamentary structures. Based on the (i) presence of filamentary
structures, (ii) distribution of cores across the region, with $\sim39$% found
along the filamentary structures, (iii) massive star-formation tracers in the
hub, and (iv) the kinematics, we believe that global hierarchical collapse can
plausibly explain the observed features in RCW 117.
