Simulations of dwarf galaxies show V/σ rising with stellar mass, with HI gas and young stars more rotation-supported than old stars.
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2026 3verdicts
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Stacked ultra-deep images of dwarf irregular galaxies reveal a pure exponential stellar disk extending to surface brightness of 32.3 mag/arcsec² without a detectable stellar halo, attributed to internal evolutionary processes.
The size-mass relation for star-forming galaxies at 0.6 < z ≤ 4 shows a gradient in slope with rest-frame wavelength, crossing at ~10^9.5 solar masses proposed as the transition between diffuse and compact morphologies.
citing papers explorer
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$V/\sigma$ Trends with Mass for Dwarf Galaxies from the Marvelous Massive Dwarfs Suite
Simulations of dwarf galaxies show V/σ rising with stellar mass, with HI gas and young stars more rotation-supported than old stars.
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Ultra-deep imaging of nearby dwarf irregular galaxies: stellar haloes and disk structure
Stacked ultra-deep images of dwarf irregular galaxies reveal a pure exponential stellar disk extending to surface brightness of 32.3 mag/arcsec² without a detectable stellar halo, attributed to internal evolutionary processes.
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CANUCS/Technicolor Data Release 2: A Catalogue of Galaxy Structural Parameters in up to 29 HST+JWST bands and a Multi-Wavelength Exploration of the Galaxy Size-Mass Relation at $0.6 < z \leq 4$
The size-mass relation for star-forming galaxies at 0.6 < z ≤ 4 shows a gradient in slope with rest-frame wavelength, crossing at ~10^9.5 solar masses proposed as the transition between diffuse and compact morphologies.