The Diffuse Ionized Gas Halo of the Small Magellanic Cloud
Author:
Funder
NSF
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
https://iopscience.iop.org/article/10.3847/1538-4357/ab4d58/pdf
Reference65 articles.
1. WARM IONIZED GAS REVEALED IN THE MAGELLANIC BRIDGE TIDAL REMNANT: CONSTRAINING THE BARYON CONTENT AND THE ESCAPING IONIZING PHOTONS AROUND DWARF GALAXIES
2. PRESENT-DAY GALACTIC EVOLUTION: LOW-METALLICITY, WARM, IONIZED GAS INFLOW ASSOCIATED WITH HIGH-VELOCITY CLOUD COMPLEX A
3. Revealing the Ionization Properties of the Magellanic Stream Using Optical Emission
4. HI4PI: a full-sky H i survey based on EBHIS and GASS
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2. H i filaments as potential compass needles? Comparing the magnetic field structure of the Small Magellanic Cloud to the orientation of GASKAP-H i filaments;Monthly Notices of the Royal Astronomical Society;2023-02-14
3. Rotation measure structure functions with higher-order stencils as a probe of small-scale magnetic fluctuations and its application to the Small and Large Magellanic Clouds;Monthly Notices of the Royal Astronomical Society;2022-10-18
4. Ionization and Star Formation in the Giant H ii Region SMC-N66;Publications of the Astronomical Society of the Pacific;2022-06-01
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