Authors: E.P.J. de Haas
The velocity rotation curve of NGC 1560 has a peculiar wiggle around 4.5 kpc. This makes it a favorable galaxy to test the diverse models trying to explain galactic dynamics, as for example CDM and MOND. I will fit NGC 1560 using the GR-Schwarzschild based `constant Lagrangian' model for galactic dynamics and compare it to other results. But first I will give a brief expose of the `constant Lagrangian' approach. At the end, I present same other fitting curves: those of galaxies F583-1, F579V1 and U11648.
Comments: 25 Pages.
[v1] 2018-04-24 09:11:00
Unique-IP document downloads: 12 times
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