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$\require{mediawiki-texvc}$ Supermassive black holes at the centre of activegalactic nuclei (AGN) produce relativistic jets that can affect the starformation characteristics of the AGN hosts. Observations in the ultraviolet(UV) band can provide an excellent view of the effect of AGN jets on starformation. Here, we present a census of star formation properties in theNorthern Star-forming Region (NSR) that spans about 20 kpc of the large radiosource Centaurus A hosted by the giant elliptical galaxy NGC 5128. In thisregion, we identified 352 UV sources associated with Cen A using newobservations at an angular resolution of $<$1.5 arcseconds observed with theUltra-Violet Imaging Telescope (UVIT) onboard AstroSat. These observations werecarried out in one far-ultraviolet (FUV; $\lambda_{\text{mean}}$ = 1481 $\AA$)and three near-ultraviolet (NUV; with $\lambda_{\text{mean}}$ of 2196 $\AA$,2447 $\AA$, and 2792 $\AA$, respectively) bands. The star-forming sourcesidentified in UV tend to lie in the direction of the jet of Cen A, therebysuggesting jet triggering of star formation. Separating the NSR into Outer andInner regions, we found the stars in the Inner region to have a relativelyyounger age than the Outer region, suggesting that the two regions may havedifferent star formation histories. We also provide the UVIT source cataloguein the NSR.

UVIT view of Centaurus A; a detailed study on positive AGN feedback