Metal and molecule cooling in simulations of structure formation

Abstract

This submission has been withdrawn by arXiv administrators because it is a duplicate of 0704.2182.

References in corpus (6)

• Wilkinson Microwave Anisotropy Probe (WMAP) Three Year Results: Implications for Cosmology
• A probable stellar solution to the cosmological lithium discrepancy
• Fragmentation of star-forming clouds enriched with the first dust
• Early structure formation in quintessence models and its implications for cosmic reionisation from first stars
• The role of HD cooling in primordial star formation
• Primordial Stellar Feedback and the Origin of Hyper Metal-Poor Stars

Cited by in corpus (25)

• The effect of photo-ionization on the cooling rates of enriched, astrophysical plasmas
• Resolving the Formation of Protogalaxies. III. Feedback from the First Stars
• Keeping the Universe ionised: Photo-heating and the clumping factor of the high-redshift intergalactic medium
• Simulating cosmic metal enrichment by the first galaxies
• Modeling the cosmological co-evolution of supermassive black holes and galaxies: I. BH scaling relations and the AGN luminosity function
• Simulation techniques for cosmological simulations
• Thermal radiation processes
• Constraining the PopIII IMF with high-z GRBs
• Photo-heating and the fate of hard photons during the reionisation of HeII by quasars
• Interpreting the evolution of galaxy colours from $z=8$ to $z=5$
• The First Billion Years of a Warm Dark Matter Universe
• The Overlooked Potential of Generalized Linear Models in Astronomy - I: Binomial Regression
• Numerical simulations of dwarf galaxy merger trees
• Dark Matter Halo Environment for Primordial Star Formation
• The effect of non-equilibrium metal cooling on the interstellar medium
• The evolution of the star formation rate function and cosmic star formation rate density of galaxies at $z\sim 1-4$
• Evolution of dust and molecular hydrogen in the Magellanic System
• Effect of Intergalactic Medium on the Observability of Lyman Alpha Emitters during Cosmic Reionization
• Formation of carbon-enhanced metal-poor stars in the presence of far ultraviolet radiation
• PopIII signatures in the spectra of PopII/I GRBs
• ROBO: a Model and a Code for the Study of the Interstellar Medium
• Simulated metal and HI absorption lines at the conclusion of Reionization
• Cosmic Star Formation: a simple model of the SFRD(z)
• Metal enrichment signatures of the first stars on high-z DLAs
• The First Billion Years project: gamma-ray bursts at z>5