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In this paper, we present the synchrotron light curve at 610 MHz from therecurrent nova V745 Sco following its outburst on 6 February 2014. The systemhas been detected and periodically monitored with the Giant Metrewave RadioTelescope (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 synchrotronemitting region obscured by foreground thermal gas which eventually becomesoptically thin to the low GMRT frequencies. We present the model fit to the2014 data on V745 Sco and discuss it alongwith the model fit to the 1.4 GHzdata of the recurrent nova RS Ophiuchi following its outburst in 1985.

Modelling the synchrotron light curves in recurrent novae V745 Scorpii and RS Ophiuchi