most citedA Fast, Hot Wind from a Nuclear Starburst

3 citations · 4 across the 5 of their papers we have counts for

collaborators

7 papers

astro-ph.GA2026

Supersonic Motion in the Driving Region of M82

Skylar Grayson, Evan Scannapieco, Philipp Grete +5

The prototypical starburst galaxy M82 is host to an expansive, multiphase outflow whose driving mechanism is not fully understood. Longstanding models suggest that energy and mass…

astro-ph.HE2026

The First Insights into an Ultraluminous X-ray Pulsar with XRISM: Phase-Resolved High-Resolution Spectroscopy of the Fe K-shell Band of M82 X-2

Shogo B. Kobayashi, Peter Kosec, Kazuki Ampuku +18

During the performance verification phase, XRISM observed the M82 galaxy for a net exposure of 207.7 ks, with the ultraluminous X-ray pulsar (ULXP) X-2 included in the field of vie…

astro-ph.GA20263 cited

A Fast, Hot Wind from a Nuclear Starburst

XRISM Collaboration, Marc Audard, Hisamitsu Awaki +137

Galaxies with intense star formation often host multiphase, galaxy-scale winds powered by supernovae and fast stellar winds. These are strong enough to disrupt the star-forming int…

astro-ph.CO2026

Kiloparsec-scale turbulence driven by reionization may grow intergalactic magnetic fields

Christopher Cain, Matthew McQuinn, Evan Scannapieco +2

The intergalactic medium (IGM) underwent intense heating that resulted in pressure disequilibrium in the wake of ionization fronts during cosmic reionization. The dynamical relaxat…

astro-ph.CO2026

Cross-correlating the patchy screening and kinetic Sunyaev-Zel'dovich effects as a new probe of reionization

Darby Kramer, Alexander van Engelen, Christopher Cain +5

The kinetic Sunyaev-Zel'dovich effect (kSZ) and patchy screening effect are two complementary cosmic microwave background (CMB) probes of the reionization era. The kSZ effect is a…

astro-ph.HE2025

XRISM constraints on unidentified X-ray emission lines, including the 3.5 keV line, in the stacked spectrum of ten galaxy clusters

XRISM Collaboration, Marc Audard, Hisamitsu Awaki +150

We stack 3.75 Megaseconds of early XRISM Resolve observations of ten galaxy clusters to search for unidentified spectral lines in the 2.5-15 keV band (rest frame), including t…