3 papers
astro-ph.GA2026
Is Milky Way gravitationally stable? A TNG50 view from cosmic noon to the present day
K. Aditya, Sandeep Kataria
We investigate the stability of Milky Way analogs (MWAs) in the \texttt{TNG50} simulation against the growth of local axisymmetric instabilities, tracing their evolution from cosmi…
astro-ph.GA2025
Can dwarf spheroidal galaxies host a central black hole ?
K. Aditya, A. Mangalam
We construct mass models of Milky Way dwarf spheroidal galaxies to place constraints on the central black hole (BH) masses they can host. We model the galaxies as a three-component…
astro-ph.GA2025
Evolution of low surface brightness ultra-thin galaxies: The role of dark matter halo and bar formation on disk thickness
K. Aditya, Arunima Banerjee
We investigate how stellar disks sustain their ultrathin structure throughout their evolution. We follow the evolution of ultrathin stellar disks with varying dark matter (DM) halo…