Cosmological simulations and galaxy formation: applications to GIRAFFE

Details Cosmological simulations and galaxy formation: applications to GIRAFFE Cosmological simulations and galaxy formation: applications to GIRAFFE

Nov 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009sf2a.conf..219p&link_type=abstract

SF2A-2009: Proceedings of the Annual meeting of the French Society of Astronomy and Astrophysics, held 29 June - 4 July 2009 in

Astronomy and Astrophysics

Astrophysics

Scientific paper

We compare the morphological and kinematic properties of massive galaxies at z=0.4-0.75 obtained by the GIRAFFE spectrograph, to those derived from the merger of two spiral galaxies described by N-body simulations, including a star formation prescription. The study of these systems is particularly interesting to the understanding of the connection between mergers and bars, as well as the properties and fate of this system in relation to disk galaxy formation.

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