Numerical hydrodynamic simulations based on semi-analytic galaxy merger trees: Method and milky way-like galaxies

Benjamin P. Moster, Andrea Maccio, Rachel S. Somerville

Research output: Contribution to journalArticle

Abstract

We present a new approach to study galaxy evolution in a cosmological context. We combine cosmological merger trees and semi-analytic models of galaxy formation to provide the initial conditions for multimerger hydrodynamic simulations. In this way, we exploit the advantages of merger simulations (high resolution and inclusion of the gas physics) and semi-analytic models (cosmological background and low computational cost), and integrate them to create a novel tool. This approach allows us to study the evolution of various galaxy properties, including the treatment of the hot gaseous halo from which gas cools and accretes on to the central disc, which has been neglected in many previous studies. This method shows several advantages over other methods. As only the particles in the regions of interest are included, the run time is much shorter than in traditional cosmological simulations, leading to greater computational efficiency. Using cosmological simulations, we show that multiple mergers are expected to be more common than sequences of isolated mergers, and therefore studies of galaxy mergers should take this into account. In this pilot study, we present our method and illustrate the results of simulating 10 Milky Way-like galaxies since z = 1. We find good agreement with observations for the total stellarmasses, star formation rates, cold gas fractions and disc scalelength parameters. We expect that this novel numerical approach will be very useful for pursuing a number of questions pertaining to the transformation of galaxy internal structure through cosmic time.

Original languageEnglish (US)
Article numberstt1702
Pages (from-to)1027-1044
Number of pages18
JournalMonthly Notices of the Royal Astronomical Society
Volume437
Issue number2
DOIs
StatePublished - Nov 1 2013

Fingerprint

Milky Way Galaxy
merger
hydrodynamics
galaxies
simulation
gas
cold gas
galactic evolution
star formation rate
gases
halos
inclusions
costs
physics
method
high resolution
cost

Keywords

  • Galaxies:Evolution
  • Galaxies:Interactions
  • galaxies:Structure
  • Galaxy:Evolution
  • Methods:Numerical

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

Numerical hydrodynamic simulations based on semi-analytic galaxy merger trees : Method and milky way-like galaxies. / Moster, Benjamin P.; Maccio, Andrea; Somerville, Rachel S.

In: Monthly Notices of the Royal Astronomical Society, Vol. 437, No. 2, stt1702, 01.11.2013, p. 1027-1044.

Research output: Contribution to journalArticle

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