Measuring Dark Matter Halos by Modeling Interacting Galaxies
2004 ◽
Vol 220
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pp. 461-462
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Keyword(s):
The richness of tidal features seen in interacting galaxies allows for the determination of their characteristic parameters, provided one can deal with the extended parameter space. Genetic algorithm based methods – like our code minga – have proven to be such a tool. Here I discuss the implementation of dark matter halo descriptions in the restricted N-body simulations of minga. I show that the final morphology of a galaxy encounter strongly depends on the halo properties. Thus, modeling tidal features of interacting galaxies might allow also for conclusions on the galactic dark matter content.
Keyword(s):
2019 ◽
Vol 55
(2)
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pp. 231-235
2009 ◽
Vol 5
(S266)
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pp. 365-365
Keyword(s):
2012 ◽
Vol 8
(S295)
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pp. 105-108
Keyword(s):
Keyword(s):
1999 ◽
Vol 183
◽
pp. 155-155
2019 ◽
Vol 487
(3)
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pp. 4025-4036
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