  In this paper, we present the synchrotron light curve at 610 MHz from the
recurrent nova V745 Sco following its outburst on 6 February 2014. The system
has been detected and periodically monitored with the Giant Metrewave Radio
Telescope (GMRT) since 9 February 2014 as part of the Galactic Nova with GMRT
(GNovaG) project. The light curves are well fit by a model of synchrotron
emitting region obscured by foreground thermal gas which eventually becomes
optically thin to the low GMRT frequencies. We present the model fit to the
2014 data on V745 Sco and discuss it alongwith the model fit to the 1.4 GHz
data of the recurrent nova RS Ophiuchi following its outburst in 1985.
