Abstract
We study resolution effects in numerical simulations of gas-rich (20% of the total baryonic mass) major mergers, and show that the formation of slowly-rotating elliptical galaxies requires a resolution that is beyond the present-day standards to be properly modelled. Our findings show that a high-enough resolution is required to accurately model the global properties of merger remnants and the evolution of their angular momentum. The role of wet mergers of spiral galaxies in the formation of slow-rotating ellipticals may therefore have been underestimated.
Original language | English |
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Title of host publication | Hunting for the Dark: The Hidden Side of Galaxy Formation - Proceedings of the International Conference |
Editors | Victor P. Debattista, Cristina C. Popescu |
Place of Publication | Melville, NY |
Publisher | American Institute of Physics |
Pages | 405-406 |
Number of pages | 2 |
Volume | 1240/1 |
ISBN (Print) | 9780735407862 |
DOIs | |
Publication status | Published - Jun 2010 |
Externally published | Yes |
Event | International Conference "Hunting for the Dark: The Hidden Side of Galaxy Formation" - Qawra, Malta Duration: 19 Oct 2009 → 23 Oct 2009 |
Other
Other | International Conference "Hunting for the Dark: The Hidden Side of Galaxy Formation" |
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Country/Territory | Malta |
City | Qawra |
Period | 19/10/09 → 23/10/09 |