collaborators

8 papers

astro-ph.HE2026

Thermal Structure and Chemical Enrichment of the North and South Polar Spurs: Supersolar N/O and Ne/O in the X-ray Plasma

Anjali Gupta, Smita Mathur, Joshua Kingsbury +5

The North Polar Spur (NPS) is a prominent diffuse X-ray feature whose origin has remained uncertain for decades. Using a uniform analysis of archival \textit{Suzaku} and \textit{XM…

astro-ph.HE2026

Not Where You Left Them: Displaced -Rays and X-Rays Reveal the Cosmic Ray Scattering Rate

Manami Roy, Mark R. Krumholz, Roland M. Crocker +1

Modern X-ray and -ray instruments are revealing a growing class of Galactic non-thermal sources whose emission centroids are measurably offset from the nearest plausible sites…

astro-ph.CO2026

Weibel Instability-Driven Seed Magnetic Fields during Reionization

Jorie McDermott, Manami Roy, Christopher M. Hirata

Cosmological reionization was a highly out-of-equilibrium event that affected every parcel of the intergalactic medium, making it a candidate for astrophysical generation of interg…

astro-ph.GA2025

To Survive or to Shatter: The Impact of Cosmic Rays on the Fate of Stripped Cold Clouds

Manami Roy, Kung-Yi Su, Stephanie Tonnesen +3

Does cosmic ray (CR) pressure matter for the circumgalactic medium (CGM)? Despite growing interest, this remains a debated question, complicated by limited observational constraint…

astro-ph.GA2025

Detection of 'super-virial' gas in the Circumgalactic medium of the Milky Way towards PKS 2155-304

Mukesh Singh Bisht, Sanskriti Das, Smita Mathur +3

We present the first simultaneous detection of four distinct highly ionized absorbing phases using Chandra and XMM-Newton grating spectra toward the blazar PKS 2155

astro-ph.GA2025

Where is the Supervirial Gas? III. Insights from X-ray Shadow Observations and a revised Model for the Soft Diffuse X-ray Background

Anjali Gupta, Smita Mathur, Joshua Kingsbury +5

Shadow observations provide a powerful tool to separate foreground components of the soft diffuse X-ray background (SDXB) from the background components. Such observations have now…