Haro 11: The Spatially Resolved Lyman Continuum Sources
As the nearest confirmed Lyman continuum (LyC) emitter, Haro 11 is an exceptional laboratory for studying LyC escape processes crucial to cosmic reionization. Our new Hubble Space Telescope/Cosmic Origins Spectrograph G130M/1055 observations of its three
Lena Komarova +15 more
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A neutral-hydrogen survey of the dwarf irregular galaxy Leo A [PDF]
N. J. Allsopp
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Dark matter search in dwarf irregular galaxies with ten years of data from the IceCube neutrino observatory [PDF]
Yi-Fei Lü +6 more
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Dwarf irregular galaxies with extended HI gas disks: Suppression of small-scale spiral structure by dark matter halo [PDF]
Soumavo Ghosh, Chanda J. Jog
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High-redshift star formation in the Atacama large millimetre/submillimetre array era. [PDF]
Hodge JA, da Cunha E.
europepmc +1 more source
Dark matter in low mass surface density galaxies
Low mass surface density spiral and irregular galaxies like low surface brightness (LSB) and dwarf galaxies are unique laboratories to study the dynamical properties of Dark Matter halos because their mass is generally dominated by dark matter at all ...
Amram, Philippe +2 more
core +1 more source
Identification of dusty massive stars in star-forming dwarf irregular galaxies in the Local Group with mid-IR photometry [PDF]
N. E. Britavskiy +4 more
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Galaxies Going Bananas: Inferring the 3D Geometry of High-redshift Galaxies with JWST-CEERS
The 3D geometries of high-redshift galaxies remain poorly understood. We build a differentiable Bayesian model and use Hamiltonian Monte Carlo to efficiently and robustly infer the 3D shapes of star-forming galaxies in James Webb Space Telescope Cosmic ...
Viraj Pandya +55 more
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Ultraviolet Imaging Telescope View of Dwarf Irregular Galaxy IC 2574: Is the Star Formation Triggered Due to Expanding H i Shells? [PDF]
Chayan Mondal +2 more
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This paper presents a quantitative analysis of the stellar content in the Local Group dwarf irregular galaxy NGC 6822 by comparing stellar evolution models and observations in color–magnitude diagrams (CMDs) and color–color diagrams (CC-Ds). Our analysis
Maria Tantalo +16 more
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