93 citations · 147 across the 10 of their papers we have counts for
10 papers
The origin of WHAM Point Source~46
S. R. Kulkarni, Zeren Lin, Charles Beichman +7
The Wisconsin H Mapper (WHAM) surveyed the entire Galactic sky in H () to approximately 0.1\,Rayleigh (R), albeit with…
Dust in the Smith Cloud? A UV Investigation into the Smith Cloud's Gas-Phase Abundance Patterns
Johanna Vazquez, Kathleen Barger, Frances Cashman +11
The Smith Cloud is a high-velocity cloud (HVC) on its final approach to the Milky Way that shows evidence of interaction with the Galaxy's disk. We investigate the metallicity and…
New Radio Observations of the Supernova Remnant CTA 1
Tam Do, Roland Kothes, Alex S. Hill +3
We present new radio images of the supernova remnant (SNR) CTA 1 at 1420 and 408 MHz, and in the 21 cm line of H I observed with the Dominion Radio Astrophysical Observatory Synthe…
Interaction Between Rogue HI Clouds and the Magnetic Field High Above the Galaxy
Bailey Forster, Tyler J. Foster, Roland Kothes +2
Observations of the Milky Way and external galaxies support the idea that large-scale magnetic fields are concentrated in galactic disks, with halo magnetic fields at least an orde…
The Diffuse Ionized Gas Halo of the Small Magellanic Cloud
Brianna M Smart, Lawrence M Haffner, Kat Barger +2
Observations with the Wisconsin H-alpha Mapper (WHAM) reveal a large, diffuse ionized halo that surrounds the Small Magellanic Cloud (SMC). We present the first kinematic H-alpha s…
Revealing the Ionization Properties of the Magellanic Stream using Optical Emission
K. A. Barger, G. J. Madsen, A. J. Fox +10
The Magellanic Stream, a gaseous tail that trails behind the Magellanic Clouds, could replenish the Milky Way with a tremendous amount of gas if it reaches the Galactic disk before…