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Dark Matter Halos around Galaxies

1 Pith paper cite this work, alongside 10 external citations. Polarity classification is still indexing.

1 Pith paper citing it
10 external citations · Pith
abstract

We present evidence that all galaxies, of any Hubble type and luminosity, bear the kinematical signature of a mass component distributed differently from the luminous matter. We review and/or derive the DM halo properties of galaxies of different luminosities and morphologies: spirals, LSBs, ellipticals, dwarf irregulars and dwarf spheroidals.

fields

cs.LG 1

years

2025 1

verdicts

CONDITIONAL 1

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