Thickness estimates of spiral galaxies

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Astrometry, Density Wave Model, Galactic Structure, Spiral Galaxies, Error Analysis, Thickness, Wave Functions

Scientific paper

A rigorous solution obtained by Tong (1981) for the perturbing potential
with a nonwavy term is used to derive the relationship between the
thickness of a spiral galaxy and the initial radius at which the arms
begin. Initial radii and, hence, average thicknesses were determined for
50 spiral galaxies.

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