activity
20232026
collaborators

5 papers

astro-ph.GA2026

Constraints on the properties of warm ionized gas from low-frequency hydrogen radio recombination lines

Pedro Salas, Kimberly L. Emig, Matteo Luisi +2

The ionized gas in the Milky Way is a major component of the interstellar medium. Observations of extinction free tracers, such as hydrogen radio recombination lines (HRRLs), have…

astro-ph.GA2026

The Impact and Environment of Massive Stars and Stellar Clusters

Loren Anderson, Jagadheep D. Pandian, Jyotirmoy Dey +10

Massive stars and stellar clusters shape galactic evolution through powerful feedback mechanisms including radiation pressure, photoionization, stellar winds, and cosmic ray accele…

astro-ph.GA2024

Implications for Galactic Electron Density Structure from Pulsar Sightlines Intersecting HII Regions

S. K. Ocker, L. D. Anderson, T. J. W. Lazio +2

Recent radio surveys have revealed pulsars with dispersion and scattering delays induced by ionized gas that are larger than the rest of the observed pulsar population, in some cas…

astro-ph.GA2024

Spectrum and polarization of the Galactic center radio transient ASKAP J173608.2-321635 from THOR-GC and VLITE

Kierra J. Weatherhead, Jeroen M. Stil, Michael Rugel +11

The radio transient ASKAP J173608.2-321735, at the position (l,b)= (356.0872,-0.0390), was serendipitously observed by The HI/OH/Recombination Line Survey of the Galactic Center (T…

astro-ph.GA2023

Turbulent Structure In Supernova Remnants G46.8-0.3 And G39.2-0.3 From THOR Polarimetry

Russell Shanahan, Jeroen Stil, Loren Anderson +5

We present the continued analysis of polarization and Faraday rotation for the supernova remnants (SNRs) G46.8-0.3 and G39.2-0.3 in L-band (1-2 GHz) radio continuum in The HI/OH/Re…