Corpus ID: 117278637

Neighboring Galaxies' Influence on Rotation Curve Asymmetry

@inproceedings{Hodge2003NeighboringGI,
  title={Neighboring Galaxies' Influence on Rotation Curve Asymmetry},
  author={John C. Hodge and Michael W. Castelaz},
  year={2003}
}
The rotation velocity asymmetry v observed in spiral galaxy HI rotation curves linearly correlates with the effective potential force from the 10 closest neighboring galaxies normalized for the test particle mass and the gravitational constant. The magnitude of the potential force from a close galaxy is proportional to the luminosity of the close galaxy and inversely proportional to the square of the distance from the close galaxy to the target galaxy. The correlation coefficient is 0.99 and F… Expand
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