The Relative Merits of Galactic Density Functions: An Orbit Computational Viewpoint

Details The Relative Merits of Galactic Density Functions: An Orbit Computational Viewpoint The Relative Merits of Galactic Density Functions: An Orbit Computational Viewpoint

Aug 1972

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1972ap%26ss..17..447i&link_type=abstract

Astrophysics and Space Science, Volume 17, Issue 2, pp.447-452

Astronomy and Astrophysics

Astrophysics

3

Scientific paper

Certain analytic functions used in galactic mass models are reviewed
from a somewhat biased orbit-computational viewpoint. On this basis, it
is argued that at the present time, and optimal galactic mass model
should be a superposition of spheroids with two kinds of density laws:
the Schmidt (1956) type, and a new type given by Equation (3).

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