  We present an ultra-violet study of two nearby dwarf irregular galaxies WLM
and IC~2574, using the Far-UV and Near-UV data from the Ultra-Violet Imaging
Telescope (UVIT). We used the F148W band Far-UV images and identified 180 and
782 young star-forming clumps in WLM and IC~2574, respectively. The identified
clumps have sizes between 7 - 30 pc in WLM and 26 - 150 pc in IC~2574. We
noticed more prominent hierarchical splitting in the structure of star-forming
regions at different flux levels in IC~2574 than WLM. We found that the
majority of the clumps have elongated shapes in the sky plane with ellipticity
($\epsilon$) greater than 0.6 in both the galaxies. The major axis of the
identified clumps is found to show no specific trend of orientation in IC~2574,
whereas in WLM the majority are aligned along south-west to north-east
direction. We estimated (F148W$-$N242W) colour for the clumps identified in WLM
and noticed that the younger ones (with (F148W$-$N242W) $<-0.5$) are smaller in
size ($<10$ pc) and are located mostly in the southern half of the galaxy
between galactocentric radii 0.4 - 0.8 kpc.
