Formation of slowly rotating elliptical galaxies in major mergers. A resolution study

M. Bois*, F. Bournaud, E. Emsellem, K. Alatalo, L. Blitz, M. Bureau, M. Cappellari, R. L. Davies, T. A. Davis, P. T. De Zeeuw, J. Falcón-Barroso, S. Khochfar, D. Krajnović, H. Kuntschner, P. Y. Lablanche, R. M. McDermid, R. Morganti, T. Naab, M. Sarzi, N. ScottP. Serra, R. C E Van Den Bosch, G. Van De Ven, A. Weijmans, L. M. Young

*Corresponding author for this work

Research output: Chapter in Book/Report/Conference proceedingConference proceeding contribution

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 languageEnglish
Title of host publicationHunting for the Dark: The Hidden Side of Galaxy Formation - Proceedings of the International Conference
EditorsVictor P. Debattista, Cristina C. Popescu
Place of PublicationMelville, NY
PublisherAmerican Institute of Physics
Pages405-406
Number of pages2
Volume1240/1
ISBN (Print)9780735407862
DOIs
Publication statusPublished - Jun 2010
Externally publishedYes
EventInternational Conference "Hunting for the Dark: The Hidden Side of Galaxy Formation" - Qawra, Malta
Duration: 19 Oct 200923 Oct 2009

Other

OtherInternational Conference "Hunting for the Dark: The Hidden Side of Galaxy Formation"
Country/TerritoryMalta
CityQawra
Period19/10/0923/10/09

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