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Over the next decade, observations conducted with ALMA and the SKA willreveal the process of mass assembly and accretion onto young stars and will berevolutionary for studies of star formation. Here we summarise the capabilitiesof ALMA and discuss recent results from its early science observations. We thenreview infrared and radio variability observations of both young low-mass andhigh-mass stars. A time domain SKA radio continuum survey of star formingregions is then outlined. This survey will produce radio light-curves forhundreds of young sources, providing for the first time a systematic survey ofradio variability across the full range of stellar masses. These light-curveswill probe the magnetospheric interactions of young binary systems, the originsof outflows, trace episodic accretion on the central sources and potentiallyconstrain the rotation rates of embedded sources.

Star and Stellar Cluster Formation: ALMA-SKA Synergies