collaborators

6 papers

astro-ph.GA2026

Radio Continuum Emission from Evolving Star-Forming Galaxies -- I. Correlations Involving the Total Synchrotron Luminosity

Sukanta Ghosh, Luke Chamandy, Charles Jose +3

Synchrotron radiation dominates the continuum emission of star-forming galaxies in the frequency range from a few to about . We model the total synchrotron…

astro-ph.GA2026

The Distribution of Cosmic Ray Electrons in Star-Forming Galaxies

Anvar Shukurov, Charles Jose

We derive explicit, algebraic expressions for the steady-state number density of cosmic ray electrons as a function of position and energy using Green's function of the diffusion e…

astro-ph.GA2026

Turbulent dynamos in a collapsing cloud

Muhammed Irshad P, Pallavi Bhat, Kandaswamy Subramanian +1

The amplification of magnetic fields is crucial for understanding the observed magnetization of stars and galaxies. Turbulent dynamo is the primary mechanism responsible for that b…

astro-ph.GA2025

The fine structure of the mean magnetic field in M31

Indrajit Paul, R. Vasanth Kashyap, Tuhin Ghosh +4

To explore the spatial variations of the regular (mean) magnetic field of the Andromeda galaxy (M31), we use Fourier analysis in azimuthal angle along four rings in the galaxy's pl…

astro-ph.GA2025

Mathematical Aspects of Geophysical and Astrophysical Fluid Dynamics: Magnetic buoyancy instability in galaxies

Yasin Qazi, Anvar Shukurov, Devika Tharakkal +1

We study the nonlinear evolution of the magnetic buoyancy instability in rotating and non-rotating gas layers using numerical solutions of non-ideal, isothermal MHD equations. The…

astro-ph.GA2025

Non-linear magnetic buoyancy instability and galactic dynamos

Yasin Qazi, Anvar. Shukurov, Frederick. A. Gent +2

Magnetic buoyancy (MBI) and Parker instabilities are strong, generic instabilities expected to occur in most astrophysical systems with sufficiently strong magnetic fields. In gala…