99 citations
- National Radio Astronomy ObservatoryUS22 papers
- West Virginia UniversityUS19 papers
- University of VirginiaUS13 papers
- Boston UniversityUS9 papers
- European Southern ObservatoryCL7 papers
- Australian National UniversityAU6 papers
- Centre National de la Recherche ScientifiqueFR6 papers
- International Centre for Radio Astronomy ResearchAU6 papers
- McGill UniversityCA6 papers
- University of PennsylvaniaUS6 papers
- Astronomy and SpaceAU5 papers
- Commonwealth Scientific and Industrial Research OrganisationAU5 papers
10 papers · 1 filter
Discovery of a New Population of Galactic HII Regions with Ionized Gas Velocity Gradients
Dana S. Balser, Trey V. Wenger, L. D. Anderson +4
We investigate the kinematic properties of Galactic HII regions using radio recombination line (RRL) emission detected by the Australia Telescope Compact Array (ATCA) at 4-10 GHz a…
Observations of compact sources in galaxy clusters using MUSTANG2
Simon R. Dicker, Elia S. Battistelli, Tanay Bhandarkar +26
Compact sources can cause scatter in the scaling relationships between the amplitude of the thermal Sunyaev-Zel'dovich Effect (tSZE) in galaxy clusters and cluster mass. Estimates…
A high-resolution view of the filament of gas between Abell 399 and Abell 401 from the Atacama Cosmology Telescope and MUSTANG-2
Adam D. Hincks, Federico Radiconi, Charles Romero +43
We report a significant detection of the hot intergalactic medium in the filamentary bridge connecting the galaxy clusters Abell 399 and Abell 401. This result is enabled by a low-…
Thermodynamic evolution of the galaxy cluster IDCS J1426.5+3508
S. Andreon, C. Romero, F. Castagna +8
We present resolved thermodynamic profiles out to 500 kpc, about , of the galaxy cluster IDCS J1426.5+3508 with 40 kpc resolution. Thanks to the combination of Su…
Neutral vs Ion Linewidths in Barnard 5: Evidence for Penetration by MHD Waves
Jaime E. Pineda, Anika Schmiedeke, Paola Caselli +4
Dense cores are the final place where turbulence is dissipated. It has been proposed from theoretical arguments that the non-thermal velocity dispersion should be narrower both for…
Stellar feedback and triggered star formation in the prototypical bubble RCW 120
Matteo Luisi, Loren D. Anderson, Nicola Schneider +17
Radiative and mechanical feedback of massive stars regulates star formation and galaxy evolution. Positive feedback triggers the creation of new stars by collecting dense shells of…