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Global trends in morphology from massive to dwarf galaxies

astro-ph.GA · 2026-06-29 · unverdicted · novelty 6.0

Galaxies become less concentrated, more asymmetric and less clumpy toward lower stellar masses, with bar fraction declining to zero near 10^8 solar masses and CAS parameters losing separating power in the dwarf regime.

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  • Global trends in morphology from massive to dwarf galaxies astro-ph.GA · 2026-06-29 · unverdicted · none · ref 244

    Galaxies become less concentrated, more asymmetric and less clumpy toward lower stellar masses, with bar fraction declining to zero near 10^8 solar masses and CAS parameters losing separating power in the dwarf regime.