activity
20242026
collaborators

6 papers

astro-ph.GA2026

Spatial Correlations of PAH, UV, H Emission and IMF - PAH Variations in the Star-Forming Complexes of NGC 628

S Amrutha, Dimitra Rigopoulou, Mousumi Das +1

We examine the spatial correlation of emission from polycyclic aromatic hydrocarbons (PAH) (3.3 m, 7.7 m, and 11.3 m) with the far-ultraviolet (FUV), near-ultraviolet (…

astro-ph.GA2025

Two Epochs of VLBI Observations of 8 KISSR Seyfert & LINER Galaxies: Suggestions of Fast and Filamentary Outflows

Preeti Kharb, Anderson Caproni, Salmoli Ghosh +4

We present here the results from a second epoch of phase-referenced VLBA observations of 8 Seyfert and LINER galaxies from the KISSR sample. These sources were chosen based on the…

astro-ph.GA2025

Dwarf-Dwarf interactions and their influence on star formation : Insights from post-merger galaxies

Rakshit Chauhan, Smitha Subramanian, Deepak A. Kudari +2

Dwarf galaxies dominate the galaxy population across all redshifts, and majority of mergers are expected to occur between them. However, the impact of dwarf-dwarf mergers on star f…

astro-ph.GA2025

A pilot method to determine the high mass end of the Stellar Initial Mass Function in galaxies using UVIT, H-MUSE observations and applied to NGC628

S Amrutha, Mousumi Das

We present a pilot method to estimate the high-mass initial mass function (IMF) across the arm, interarm, and spur regions in galaxies and apply it to NGC 628. We extracted star-fo…

astro-ph.HE2025

First Search for High-Energy Neutrino Emission from Galaxy Mergers

Subhadip Bouri, Priyank Parashari, Mousumi Das +1

The exact sources of high-energy neutrinos detected by the IceCube neutrino observatory still remain a mystery. For the first time, this work explores the hypothesis that galaxy me…

astro-ph.GA2024

Tracing Hierarchical Star Formation out to Kiloparsec Scales in Nearby Spiral Galaxies with UVIT

Gairola Shashank, Smitha Subramanian, Sreedevi M. +5

Molecular clouds fragment under the action of supersonic turbulence & gravity which results in a scale-free hierarchical distribution of star formation (SF) within galaxies. Recent…