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This submission has been withdrawn by arXiv administrators because it is a duplicate of 0704.2182.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 (39)

• Wilkinson Microwave Anisotropy Probe (WMAP) Three Year Results: Implications for Cosmology
• The cosmological simulation code GADGET-2
• Cosmological SPH simulations: A hybrid multi-phase model for star formation
• GADGET: A code for collisionless and gasdynamical cosmological simulations
• In the Beginning: The First Sources of Light and the Reionization of the Universe
• The Formation of the First Stars. I. The Primordial Star Forming Cloud
• Equation of State of the Photoionized Intergalactic Medium
• Forming the First Stars in the Universe: The Fragmentation of Primordial Gas
• Simulations of Early Structure Formation: Primordial Gas Clouds
• Modelling Primordial Gas in Numerical Cosmology
• Formation of Primordial Stars in a LCDM Universe
• The Formation of the First Low-Mass Stars From Gas With Low Carbon and Oxygen Abundances
• The early star generations: the dominant effect of rotation on the CNO yields
• The Deuterium Abundance Towards Q1009+2956
• The First Cosmic Structures and their Effects
• A probable stellar solution to the cosmological lithium discrepancy
• The Structure and Dynamical Evolution of Dark Matter Halos
• Fragmentation of star-forming clouds enriched with the first dust
• Cosmological Hydrodynamics with Multi-Species Chemistry and Nonequilibrium Ionization and Cooling
• Low-Mass Relics of Early Star Formation
• GCD+: A New Chemodynamical Approach to Modeling SNe and Chemical Enrichment
• A New Measurement of the Primordial Abundance of Deuterium: Toward Convergence with the Baryon Density from the CMB?
• The Deuterium to Hydrogen Abundance Ratio Towards the QSO SDSS1558-0031
• Thermal Conduction in Simulated Galaxy Clusters
• Simulating the metal enrichment of the ICM
• Critical Metallicity and Fine-Structure Emission of Primordial Gas Enriched by the First Stars
• The Stellar Initial Mass Function in Primordial Galaxies
• Radiative feedback from an early X-ray background
• Reionisation, chemical enrichment and seed black holes from the first stars: is Population III important?
• The cooling function of HD molecule revisited
• Element Synthesis in Stars
• Deuterium chemistry in the primordial gas
• Early structure formation in quintessence models and its implications for cosmic reionisation from first stars
• Rate Coefficient for H^+ + H_2(X ^1Sigma_g^+, nu=0, J=0) --> H(1s) + H_2^+ Charge Transfer and Some Cosmological Implications
• Metal enrichment of the intergalactic medium
• The role of HD cooling in primordial star formation
• Primordial Stellar Feedback and the Origin of Hyper Metal-Poor Stars
• Formation of HD molecules in merging dark matter haloes
• 0103-72.6: A New Oxygen-Rich Supernova Remnant in the Small Magellanic Cloud

Cited by in corpus (121)

• The effect of photo-ionization on the cooling rates of enriched, astrophysical plasmas
• The First Galaxies
• Resolving the Formation of Protogalaxies. III. Feedback from the First Stars
• KROME - a package to embed chemistry in astrophysical simulations
• Keeping the Universe ionised: Photo-heating and the clumping factor of the high-redshift intergalactic medium
• The transition from population III to population II-I star formation
• The First Billion Years project - III: The impact of stellar radiation on the coevolution of Populations II and III
• The UV continua and inferred stellar populations of galaxies at z ~ 7 - 9 revealed by the Hubble Ultra Deep Field 2012 campaign
• Formation of Isolated Dwarf Galaxies with Feedback
• The First Supernova Explosions: Energetics, Feedback, and Chemical Enrichment
• The dust mass in z > 6 normal star forming galaxies
• Simulating cosmic metal enrichment by the first galaxies
• The Dynamical and Chemical Evolution of Dwarf Spheroidal Galaxies
• Modeling the cosmological co-evolution of supermassive black holes and galaxies: I. BH scaling relations and the AGN luminosity function
• The interplay between chemical and mechanical feedback from the first generation of stars
• Carbon-enhanced metal-poor stars in dwarf galaxies
• The assembly of dusty galaxies at $z\ge 4$: statistical properties
• The impact of primordial supersonic flows on early structure formation, reionization and the lowest-mass dwarf galaxies
• Simulation techniques for cosmological simulations
• The CoDECS project: a publicly available suite of cosmological N-body simulations for interacting dark energy models
• The Dynamical and Chemical Evolution of Dwarf Spheroidal Galaxies with GEAR
• Non-equilibrium chemistry and cooling in the diffuse interstellar medium - I. Optically thin regime
• Legacy of star formation in the pre-reionization universe
• Population III stars and the Long Gamma Ray Burst rate
• Physical Processes in Star Formation
• Thermal radiation processes
• Strong constraints on decay and annihilation of dark matter from heating of gas-rich dwarf galaxies
• Simulating the assembly of galaxies at redshifts z = 6 - 12
• Gas-rich dwarf galaxies as a new probe of dark matter interactions with ordinary matter
• Constraining the PopIII IMF with high-z GRBs
• Galactic Center Gas Clouds and Novel Bounds on Ultra-Light Dark Photon, Vector Portal, Strongly Interacting, Composite, and Super-Heavy Dark Matter
• Photo-heating and the fate of hard photons during the reionisation of HeII by quasars
• Simulating high-z Gamma-ray Burst host galaxies
• Calorimetric Dark Matter Detection With Galactic Center Gas Clouds
• Interpreting the evolution of galaxy colours from $z=8$ to $z=5$
• Observing simulated galaxy clusters with PHOX: a novel X-ray photon simulator
• Stellar orbits and the survival of metallicity gradients in simulated dwarf galaxies
• Fragmentation in the First Galaxies
• First stars in Damped Lyman Alpha systems
• The First Billion Years of a Warm Dark Matter Universe
• A radio jet drives a molecular and atomic gas outflow in multiple regions within one square kiloparsec of the nucleus of the nearby galaxy IC5063
• Detectability of the First Cosmic Explosions
• Probing the stellar initial mass function with high-$z$ supernovae
• Enrichment of the hot intracluster medium: numerical simulations
• A needle in a haystack? Catching Pop III stars in the Epoch of Reionization: I. Pop III star forming environments
• Simulations of the formation and evolution of isolated dwarf galaxies - II. Angular momentum as a second parameter
• RAMSES-RTZ: Non-Equilibrium Metal Chemistry and Cooling Coupled to On-The-Fly Radiation Hydrodynamics
• The onset of star formation in primordial haloes
• A chemical model for the interstellar medium in galaxies
• CRASH3: cosmological radiative transfer through metals
• Origin of Cosmic Chemical Abundances
• The Overlooked Potential of Generalized Linear Models in Astronomy - I: Binomial Regression
• JWST high-z galaxy constraints on warm and cold dark matter models
• Dark Matter Halo Environment for Primordial Star Formation
• Numerical simulations of dwarf galaxy merger trees
• 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 $z\sim 1-4$
• Baryon history and cosmic star formation in non-Gaussian cosmological models: numerical simulations
• Simulations of galactic disks including a dark baryonic component
• Evolution of dust and molecular hydrogen in the Magellanic System
• Simulated star formation rate functions at z~4-7, and the role of feedback in high-z galaxies
• Effect of Intergalactic Medium on the Observability of Lyman Alpha Emitters during Cosmic Reionization
• Robust PCA and MIC statistics of baryons in early mini-haloes
• Effects Of Circum-nuclear Disk Gas Evolution And The Spin Of Central Black Holes
• New composition dependent cooling and heating curves for galaxy evolution simulations
• Cosmological DCBH formation sites hostile for their growth
• Counts of high-redshift GRBs as probe of primordial non-Gaussianities
• Galactic Gas Flows from Halo to Disk: Tomography and Kinematics at the Milky Way's Disk-Halo Interface
• Chemistry of heavy elements in the Dark Ages
• Statistical properties of mass, star formation, chemical content and rotational patterns in early z > 9 structures
• Formation of carbon-enhanced metal-poor stars in the presence of far ultraviolet radiation
• Radiative feedback and cosmic molecular gas: the role of different radiative sources
• Atomic and molecular gas from the epoch of reionization down to redshift 2
• Radiative feedback and cosmic molecular gas: numerical method
• The degeneracy between star-formation parameters in dwarf galaxy simulations and the Mstar-Mhalo relation
• The seeds of supermassive black holes and the role of local radiation and metal spreading
• Gas distribution, metal enrichment, and baryon fraction in Gaussian and non-Gaussian universes
• PopIII signatures in the spectra of PopII/I GRBs
• The First Billion Years project: dark matter haloes going from contraction to expansion and back again
• ROBO: a Model and a Code for the Study of the Interstellar Medium
• Simulated metal and HI absorption lines at the conclusion of Reionization
• Atomic and molecular gas as traced by [C II] emission
• Complexity reduction of astrochemical networks
• Simulating extremely metal-poor gas and DLA metal content at redshift z=7
• The post-infall evolution of a satellite galaxy
• The effect of gravitational tides on dwarf spheroidal galaxies
• A hide-and-seek game: Looking for Population III stars during the Epoch of Reionization through the HeII$\lambda$1640 line
• The imprint of cosmological non-Gaussianities on primordial structure formation
• Developing a self-consistent AGB wind model: I. Chemical, thermal, and dynamical coupling
• Cosmic Star Formation: a simple model of the SFRD(z)
• Influence of baryonic physics in galaxy simulations: a semi-analytic treatment of the molecular component
• Neural networks: solving the chemistry of the interstellar medium
• ColdSIM predictions of [C II] emission in primordial galaxies
• Metal enrichment signatures of the first stars on high-z DLAs
• Impact of H${}_2$-driven star formation and stellar feedback from low-enrichment environments on the formation of spiral galaxies
• The First Billion Years project: gamma-ray bursts at z>5
• Massive black hole formation in Population III star clusters
• Signatures of very massive stars: supercollapsars and their cosmological rate
• Cosmological interpretation of the color-magnitude diagrams of galaxy clusters
• Carbon envelopes around merging galaxies at z ~ 4.5
• Radiative transfer of ionizing radiation through gas and dust: grain charging in star forming regions
• Hard X-ray Emission from Sh2-104: A NuSTAR search for Gamma-ray Counterparts
• Modelling thermochemical processes in protoplanetary disks I: numerical methods
• Chemical enrichment in groups and clusters
• Modelling H${}_2$ and its effects on star formation using a joint implementation of GADGET-3 and KROME
• The Degeneracy of Galaxy Formation Models
• Formation of the First Galaxies: Theory and Simulations
• Mapping Synthetic Observations to Prestellar Core Models: An Interpretable Machine Learning Approach
• LAAT: Locally Aligned Ant Technique for discovering multiple faint low dimensional structures of varying density
• Hydrodynamical chemistry simulations of the SZ effect and the impacts from primordial non-Gaussianities
• Evolution of cold streams in hot gaseous halos
• The Milky Way satellite galaxy Leo T: A perturbed cored dwarf
• Upper Limit on Star Formation and Metal Enrichment in Minihalos
• Carbon Cations and Silicon Atoms in the ISM: modeling their charge exchange reaction
• High$-z$ [OI] emission lines: ColdSIM simulations and ALMA observations
• Low-temperature primordial gas in merging halos
• Self-sustaining star formation fronts in filaments during cosmic dawn
• Origin of Weak MgII and Higher Ionization Absorption Lines in an Outflow from an Intermediate-Redshift Dwarf Satellite Galaxy
• Can UVB variations reconcile simulated quasar absorption lines at high redshift?
• The Baryon Budget of Galaxies across the First Billion Years
• HI and H${}_2$ gas evolution over cosmic times: ColdSIM