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Cite Publication Date: Aug 1, 2006 |
Affiliation: Astronomical Observatory, Osservatorio Astronomico di Padova
AbstractThe growth and the evolution of the bar instability in stellar-gaseous disks embedded in a dark matter halo evolving in a cosmological framework is explored. We point out the impact of different gas fractions on the bar formation, inside disks of different disk-to-halo mass ratio.
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