Chemodynamical simulations of galaxies from Milky Way to early-type galaxies

speaker of the seminars of the Astronomical Observatory and Physics and Astronomy Department

  • Data: 03 dicembre 2015 dalle 14:00 alle 15:00

  • Luogo: Seminars’ room, floor -1, via Ranzani 1

Contatto di riferimento:

Partecipanti: Chiaki Kobayashi (Centre for Astrophysics Research, University of Hertfordshire, UK)

Abstract



Star formation and chemical enrichment histories of galaxies are imprinted in

their internal structures of galaxies, i.e., kinematics and elemental

abundances of stars within galaxies. We predict the distribution of elements

within galaxies using our chemodynamical simulations. In the simulated Milky

Way-type galaxies, the bulge formed though assembly of gas-rich galaxies at

high-redshifts, and has old, metal-rich, and alpha-enhanced populations. The

disk formed inside-out over Cosmic time, producing [alpha/Fe]-[Fe/H] relations.

A half of thick disk stars have formed in satellite galaxies. In each

component, the scatter in elemental abundance ratios is caused by this

accretion as well as migration and in-situ variation of chemical enrichment.

In cosmological simulations, the feedback from active galactic nuclei (AGN)

plays an essential role in questing star formation in massive galaxies and

re-distributing metals into the intergalactic medium. We have applied a new AGN

model for the formation of black holes motivated by the first star formation,

in contrast to the merging scenario of previous works. Our simulations

reproduce the observed cosmic star formation rates, black hole mass-galaxy mass

relation, size-mass relation, and mass-metallicity relation of galaxies, and

are in better agreement with the observed down-sizing phenomena, namely, the

alpha enhancement of early-type galaxies. We also predict the time evolution of

these relations and the metallicity radial gradients. At present, stellar

metallicity gradients dramatically evolve depending on their merging histories,

while gas-phase metallicity gradients are more sensitive to the AGN feedback.

 

See you on thursday in the seminars’ room, floor -1, via Ranzani 1, on time at 14:00.

Next seminars:

* Thursday December 10th, at 14:00 Corrado Boeche (University of Heidelberg, DE)

* Wednesday December 16th, at 14:00 Rodrigo Ibata (Observatoire de Strasbourg, FR)

* Thursday December 17th, at 14:00 Elena M. Rossi (Leiden Univ., NL)

 

The complete list of seminars is available at: http://davide2.bo.astro.it/?page_id=4531

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