University of Birmingham > Talks@bham > Astrophysics Seminars > Chemodynamical simulations of galaxies

  Browse A-Z

Log in

System Admin (disabled)details Birmingham usersdetails No account?details

Information on

Subscribing to talksdetails Finding a talkdetails Adding a talkdetails Disseminating talksdetails Help and Documentationdetails

Chemodynamical simulations of galaxies

Add to your list(s) Download to your calendar using vCal

If you have a question about this talk, please contact Alastair Sanderson.

The formation and evolutionary history of galaxies are imprinted in the elemental abundance ratios of stars. I am simulating the chemodynamical evolution of galaxies using my hydrodynamical code that includes star formation and chemical enrichment from core-collapse and Type Ia supernovae, and AGB stars. It is possible to predict the time/redshift evolution of the spatial distribution of elements in the Universe and to compare with observations of nearby and distant galaxies. In this talk, I will discuss the mass-metallicity relation of galaxies, the stellar populations of the Galactic bulge and disk, and the elemental abundances of metal-poor Damped Lyman alpha systems.

This talk is part of the Astrophysics Seminars series.

Tell a friend about this talk:

This talk is included in these lists:

Note that ex-directory lists are not shown.

Other lists

Met and Mat Seminar Series Analysis seminar Type the title of a new list here

Other talks

Algebraic and combinatorial decompositions of Fuchsian groups Evaluation of sources of intelligence using a multi-armed bandit framework RSC S F Boys-A Rahman Award Lecture Physics at van der Waals interfaces: Twists, incommensurability and emergent phenomena TBA The Leech Lattice and the Conway Groups
 

Talks@bham, University of Birmingham. Contact Us | Help and Documentation | Privacy and Publicity.
talks@bham is based on talks.cam from the University of Cambridge.