HYDRODYNAMICAL SIMULATIONS OF GALAXY CLUSTERS WITH GALCONS
- School of Physics and Astronomy, Tel Aviv University, Tel Aviv 69978 (Israel)
- Center for Astrophysics and Space Sciences, University of California, San Diego, La Jolla, CA 92093-0424 (United States)
We present our recently developed galcon approach to hydrodynamical cosmological simulations of galaxy clusters-a subgrid model added to the Enzo adaptive mesh refinement code-which is capable of tracking galaxies within the cluster potential and following the feedback of their main baryonic processes. Galcons are physically extended galactic constructs within which baryonic processes are modeled analytically. By identifying galaxy halos and initializing galcons at high redshift (z {approx} 3, well before most clusters virialize), we are able to follow the evolution of star formation (SF), galactic winds, and ram pressure stripping of interstellar media, along with their associated mass, metals, and energy feedback into intracluster (IC) gas, which are deposited through a well-resolved spherical interface layer. Our approach is fully described and all results from initial simulations with the enhanced Enzo-Galcon code are presented. With a galactic SF rate derived from the observed cosmic SF density, our galcon simulation better reproduces the observed properties of IC gas, including the density, temperature, metallicity, and entropy profiles. By following the impact of a large number of galaxies on IC gas we explicitly demonstrate the advantages of this approach in producing a lower stellar fraction, a larger gas core radius, an isothermal temperature profile in the central cluster region, and a flatter metallicity gradient than in a standard simulation.
- OSTI ID:
- 21452948
- Journal Information:
- Astrophysical Journal, Vol. 716, Issue 2; Other Information: DOI: 10.1088/0004-637X/716/2/918; ISSN 0004-637X
- Country of Publication:
- United States
- Language:
- English
Similar Records
FORMING REALISTIC LATE-TYPE SPIRALS IN A {Lambda}CDM UNIVERSE: THE ERIS SIMULATION
GALAXY CLUSTERS AT THE EDGE: TEMPERATURE, ENTROPY, AND GAS DYNAMICS NEAR THE VIRIAL RADIUS