I have been working on numerical modeling of Active Galactic Nuclei and its observational verification, physics of Inter Stellar Medium, galactic dynamics/structures and formation of supermassive black holes.
I have been studying the dynamics, formation and evolution of galaxies from low to high redshifts with simulations and analytic approaches.
Keywords: cosmological simulation, disc instability, spiral arm, giant clump, dark matter halo, line-emission modelling.
I am a postdoctoral researcher. I am interested in the physical and chemical processes around the stellar surface and the circumstellar envelope of evolved giants. Now I am constructing the numerical code for MHD wind models from evolved giants including the effects of stellar pulsation and turbulent pressure.
I am an Indian PhD student studying star forming clouds. Currently I am investigating the effects of magnetic fields in cloud cloud collision in order to better understand massive star formation. This work is done using magneto-hydrodyamical(MHD) simulations.
I study the star formation in barred spiral galaxies in simulations. Recent observations of barred spiral galaxies suggest that it is more difficult to form stars in bar regions than in spiral regions. I am trying to explain this with my models and comparing with observations.