Chemical Signature of Gas-rich disc-disc Mergers at high Redshift

We performed numerical simulations of mergers between gas-rich disc galaxies, which result in the formation of late-type galaxies. Stars formed during the merger end up in a thick disc that is partially supported by velocity dispersion and has high [α/Fe] ratios at all metallicities. Stars formed la...

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Veröffentlicht in:	Proceedings of the International Astronomical Union 2010-12, Vol.6 (S277), p.250-254
Hauptverfasser:	Martel, Hugo, Richard, Simon, Brook, Chris B., Kawata, Daisuke, Gibson, Brad K., Sánchez-Blázquez, Patricia
Format:	Artikel
Sprache:	eng
Schlagworte:	Accretion disks Chemicals Contributed Papers Gases Numerical analysis Simulation
Online-Zugang:	Volltext
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