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Rotation Curves of Spiral Galaxies

3 Pith papers cite this work. Polarity classification is still indexing.

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abstract

Rotation curves of spiral galaxies are the major tool for determining the distribution of mass in spiral galaxies. They provide fundamental information for understanding the dynamics, evolution and formation of spiral galaxies. We describe various methods to derive rotation curves, and review the results obtained. We discuss the basic characteristics of observed rotation curves in relation to various galaxy properties, such as Hubble type, structure, activity, and environment.

fields

hep-ph 2 gr-qc 1

years

2025 3

verdicts

UNVERDICTED 3

representative citing papers

Probing Heavy Dark Matter in Red Giants

hep-ph · 2025-09-03 · unverdicted · novelty 7.0

Red-giant luminosity observations at the tip of the branch are used to set upper limits on dark-matter masses near 10^11 GeV and spin-independent cross sections near 10^{-37} cm² by requiring that DM-induced core heating does not cause premature helium ignition.

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