collaborators

23 papers

astro-ph.HE2026

Can We Find the Emission Mechanism Behind the Extremely Bright GRB 230812B?

Utkarsh Pathak, Sameer K. Patil, Hitesh Tanenia +23

GRB 230812B is a bright long-duration GRB with a luminous, long-lived afterglow and an AstroSat/CZTI polarization measurement during the prompt phase, enabling a joint study of its…

astro-ph.GA2026

Caught in the act: interaction-driven evolution in the nearby compact galaxy group Roberts Quartet (SCG0018-4854)

Saili Keshri, Sudhanshu Barway, Mousumi Das +1

We present a spatially resolved multiwavelength study of the compact galaxy group Roberts Quartet (RQ, SCG0018-4854), aimed at understanding interaction-driven galaxy evolution in…

astro-ph.GA2026

Investigating the Spectral Properties of Dual Nuclei in Galaxy Mergers from the GOTHIC survey: Supermassive Black Hole Growth, metal enrichment and Dual AGN

Prerana Biswas, Mousumi Das, Sudhanshu Barway +4

Dual nuclei systems are galaxy merger remnants or closely merging galaxies that have two distinct stellar cores separated by ~ 10pc to 10kpc. They are important laboratories for pr…

astro-ph.GA2026

Cluster-centric trends in bar size and pattern speed: the case of Abell 2199

Chandan Watts, Sudhanshu Barway, Mousumi Das +1

We investigate how the environment of a dynamically unrelaxed galaxy cluster influences the structure and dynamics of stellar bars. In particular, we examine cluster-centric variat…

astro-ph.GA2026

Dwarf and Intermediate-Mass Galaxies in MaNGA: Evidence for Different Evolutionary Trends

Chandan Watts, Gothai L, Sudhanshu Barway

We investigate the interplay between morphology, specific star formation rate (sSFR), and local environment using a sample of 7,408 galaxies from the SDSS-IV MaNGA survey. Our anal…

astro-ph.GA2026

Exploring the stellar streams and satellites around the giant low surface brightness galaxy Malin 1

Roy O. E. Bustos-Espinoza, Matias Blaña, Gaspar Galaz +7

Context. Giant Low Surface Brightness galaxies, such as Malin 1, host extended discs exceeding 100 kpc. Their formation and evolution remain debated, with interactions with satelli…