Simulations of dwarf galaxies show V/σ rising with stellar mass, with HI gas and young stars more rotation-supported than old stars.
and de los Reyes, Mithi A
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
fields
astro-ph.GA 2years
2026 2verdicts
UNVERDICTED 2representative citing papers
Analysis of 3 million HSC galaxies finds that galaxy bulge-to-total ratio depends on environment at fixed stellar mass, with the strength and scale of this dependence varying by redshift and galaxy mass.
citing papers explorer
-
$V/\sigma$ 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.
-
Environmental Sculpting of Galaxy Structure at Fixed Stellar Mass: A Multi-Scale Analysis Across Cosmic Time using 3 Million HSC Galaxies
Analysis of 3 million HSC galaxies finds that galaxy bulge-to-total ratio depends on environment at fixed stellar mass, with the strength and scale of this dependence varying by redshift and galaxy mass.