Filaments in the southern giant lobe of Centaurus A: constraints on nature and origin from modelling and GMRT observations

We present results from imaging of the radio filaments in the s outhern giant lobe of Centaurus A using data from GMRT observations at 325 and 235 MHz, andoutcomes from filament modelling. The observations reveal a rich filamentary struc ture, largely matching the morphology at 1.4 GHz. We find no clear connection of the filaments to th e jet. We seek to constrain the nature and origin of the vertex and vortex filaments associated with the lobe and their role in high-energy particle acceleration. We deduce that these filaments are at most mildly overpressured with respect to the global lobe plasma showing no evidence of large-scale efficient Fermi I-type particle acceleration, and persist for � 2 3 Myr. We demonstrate that the dwarf galaxy KK 196 (AM 1318‐444) cannot account for the features, and that surface plasma instabilities, the internal sausage mode and radiative instabil ities are highly unlikely. An internal tearing instability and the kink mode are allowed within the observational and growth time constraints and could develop in parallel on different physical scales. We interpret the origin of the vertex and vortex filaments in terms of weak shocks from transonic MHD turbulen ce or from a moderately recent jet activity of the parent AGN, or an interplay of both.