The quiescent phase of galactic disc growth
We perform a series of controlled N-body simulations of growing disc galaxies within non-growing, live dark matter haloes of varying mass and concentration. Our initial conditions include either a low-mass disc or a compact bulge. New stellar particles are continuously added on near-circular orbits...
Κύριοι συγγραφείς: | , , |
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Μορφή: | Journal article |
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Oxford University Press
2015
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