The star formation main sequence and stellar mass assembly of galaxies in the Illustris simulation

Abstract

Understanding the physical processes that drive star formation is a key challenge for galaxy formation models. In this article we study the tight correlation between the star formation rate (SFR) and stellar mass of galaxies at a given redshift, how halo growth influences star formation, and star formation histories of individual galaxies. We study these topics using Illustris, a state-of-the-art cosmological hydrodynamical simulation of galaxy formation. Illustris reproduces the observed relation (the star formation main sequence; SFMS) between SFR and stellar mass at redshifts z=0 and z=4, but at intermediate redshifts of z~2, the simulated SFMS has a significantly lower normalisation than reported by observations. The scatter in the relation is consistent with the observed scatter. However, the fraction of outliers above the SFR-stellar mass relation in Illustris is less than that observed. Galaxies with halo masses of ~10^{12} solar masses dominate the SFR density of the Universe, in agreement with the results of abundance matching. Furthermore, more-massive galaxies tend to form the bulk of their stars at high redshift, which indicates that `downsizing' occurs in Illustris. We also studied the star formation histories of individual galaxies, including the use of a principal component analysis decomposition. We find that for fixed stellar mass, galaxies that form earlier have more-massive black holes at z=0, indicating that star formation and black hole growth are tightly linked processes in Illustris. While many of the properties of normal star-forming galaxies are well-reproduced in the Illustris simulation, forming a realistic population of starbursts will likely require higher resolution and probably a more sophisticated treatment of star formation and feedback from stars and black holes.

16 pages, 16 figures, Accepted for MNRAS, Section 6 and Figure 16 are new. Data is available at http://martinsparre.com/dataproducts

References in corpus (100)

• Galactic Stellar and Substellar Initial Mass Function
• The Global Schmidt Law in Star Forming Galaxies
• Nine-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Parameter Results
• Simulating the joint evolution of quasars, galaxies and their large-scale distribution
• The EAGLE project: Simulating the evolution and assembly of galaxies and their environments
• The Origin of the Mass--Metallicity Relation: Insights from 53,000 Star-Forming Galaxies in the SDSS
• The physical properties of star forming galaxies in the low redshift universe
• Star Formation in the Milky Way and Nearby Galaxies
• E pur si muove: Galiliean-invariant cosmological hydrodynamical simulations on a moving mesh
• Cosmological SPH simulations: A hybrid multi-phase model for star formation
• Introducing the Illustris Project: Simulating the coevolution of dark and visible matter in the Universe
• Modeling feedback from stars and black holes in galaxy mergers
• The Average Star Formation Histories of Galaxies in Dark Matter Halos from z=0-8
• On the normalisation of the cosmic star formation history
• Cold streams in early massive hot haloes as the main mode of galaxy formation
• Gasdynamics and Starbursts in Major Mergers
• UV Star Formation Rates in the Local Universe
• Color Separation of Galaxy Types in the Sloan Digital Sky Survey Imaging Data
• Multiwavelength study of massive galaxies at z~2. I. Star formation and galaxy growth
• A Highly Consistent Framework for the Evolution of the Star-Forming "Main Sequence" from z~0-6
• Galaxies on FIRE (Feedback In Realistic Environments): Stellar Feedback Explains Cosmologically Inefficient Star Formation
• Galactic star formation and accretion histories from matching galaxies to dark matter haloes
• The Star Formation History of Field Galaxies
• Properties of galaxies reproduced by a hydrodynamic simulation
• The CANADA-FRANCE REDSHIFT SURVEY XIII: The luminosity density and star-formation history of the Universe to z ~ 1
• GOODS-Herschel: an infrared main sequence for star-forming galaxies
• Galaxy Luminosity Functions to z~1: DEEP2 vs. COMBO-17 and Implications for Red Galaxy Formation
• A fundamental relation between mass, SFR and metallicity in local and high redshift galaxies
• Introducing the Illustris Project: the evolution of galaxy populations across cosmic time
• At the heart of the matter: the origin of bulgeless dwarf galaxies and Dark Matter cores
• Formation of Massive Galaxies at High Redshift: Cold Streams, Clumpy Disks and Compact Spheroids
• A model for cosmological simulations of galaxy formation physics
• A Study of the Gas-Star Formation Relation over Cosmic Time
• Halos and galaxies in the standard cosmological model: results from the Bolshoi simulation
• The Star-formation Mass Sequence out to z=2.5
• A unified model for AGN feedback in cosmological simulations of structure formation
• Clumps and streams in the local dark matter distribution
• Gas-regulation of galaxies: the evolution of the cosmic sSFR, the metallicity-mass-SFR relation and the stellar content of haloes
• The lesser role of starbursts for star formation at z=2
• The physics driving the cosmic star formation history
• Different star formation laws for disks versus starbursts at low and high redshifts
• Galaxy Structure and Mode of Star Formation in the SFR-Mass Plane from z ~ 2.5 to z ~ 0.1
• The Green Valley is a Red Herring: Galaxy Zoo reveals two evolutionary pathways towards quenching of star formation in early- and late-type galaxies
• The star formation history of mass-selected galaxies in the COSMOS field
• The Impact of cold gas accretion above a mass floor on galaxy scaling relations
• On the evolution of star forming galaxies
• Forming Realistic Late-Type Spirals in a LCDM Universe: The Eris Simulation
• An Analytic Model for the Evolution of the Stellar, Gas, and Metal Content of Galaxies
• The effect of galaxy mass ratio on merger--driven starbursts
• Star formation efficiency in galaxy interactions and mergers: a statistical study
• Star formation in AEGIS field galaxies since z=1.1 . Staged galaxy formation, and a model of mass-dependent gas exhaustion
• Moving mesh cosmology: tracing cosmological gas accretion
• The formation of disc galaxies in high resolution moving-mesh cosmological simulations
• Galaxy Evolution in Cosmological Simulations With Outflows I: Stellar Masses and Star Formation Rates
• A physical model for cosmological simulations of galaxy formation: multi-epoch validation
• The galaxy stellar mass-star formation rate relation: Evidence for an evolving stellar initial mass function?
• Toy Models for Galaxy Formation versus Simulations
• Sub-millimeter galaxies as progenitors of compact quiescent galaxies
• The contribution of starbursts and normal galaxies to infrared luminosity functions at z < 2
• The Star Formation Rate Density and Dust Attenuation Evolution over 12 Gyr with the VVDS Surveys
• On the frequency, intensity and duration of starburst episodes triggered by galaxy interactions and mergers
• Galaxy Pairs in the Sloan Digital Sky Survey - V. Tracing changes in star formation rate and metallicity out to separations of 80 kpc
• On the Lack of Evolution in Galaxy Star Formation Efficiency
• Galaxy pairs in the Sloan Digital Sky Survey - VI. The orbital extent of enhanced star formation in interacting galaxies
• A unified empirical model for infrared galaxy counts based on observed physical evolution of distant galaxies
• Galaxy growth in the concordance $\Lambda$CDM cosmology
• Simulations of the galaxy population constrained by observations from z=3 to the present day: implications for galactic winds and the fate of their ejecta
• The Metallicity Evolution of Interacting Galaxies
• What Does a Submillimeter Galaxy Selection Actually Select? The Dependence of Submillimeter Flux Density on Star Formation Rate and Dust Mass
• The bright end of the galaxy luminosity function at z ~ 7: before the onset of mass quenching?
• Moving mesh cosmology: numerical techniques and global statistics
• Star formation rates and stellar masses of z=7-8 galaxies from IRAC observations of the WFC3/IR ERS and the HUDF field
• The stellar masses and specific star-formation rates of submillimetre galaxies
• Subsonic turbulence in smoothed particle hydrodynamics and moving-mesh simulations
• Halo Mass and Assembly History Exposed in the Faint Outskirts: the Stellar and Dark Matter Haloes of Illustris Galaxies
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• Moving mesh cosmology: the hydrodynamics of galaxy formation
• An analytic solution for the minimal bathtub toy model: challenges in the star-formation history of high-z galaxies
• Mergers, AGN, and 'Normal' Galaxies: Contributions to the Distribution of Star Formation Rates and Infrared Luminosity Functions
• SMA Imaging of CO(3-2) Line and 860 micron Continuum of Arp 220 : Tracing the Spatial Distribution of Luminosity
• The total infrared luminosity may significantly overestimate the star formation rate of recently quenched galaxies
• Moving mesh cosmology: characteristics of galaxies and haloes
• Damped Lyman-alpha absorbers as a probe of stellar feedback
• How to distinguish starbursts and quiescently star-forming galaxies: The `bimodal' submillimetre galaxy population as a case study
• Should we believe the results of UV-mm galaxy SED modelling?
• The redshift-evolution of the distribution of star formation among dark matter halos as seen in the infrared
• Understanding the Structural Scaling Relations of Early-Type Galaxies
• Galaxy mergers on a moving mesh: a comparison with smoothed-particle hydrodynamics
• Evolution of violent gravitational disc instability in galaxies: Late stabilization by transition from gas to stellar dominance
• Faint dwarfs as a test of DM models: WDM vs. CDM
• Determining the stellar masses of submillimetre galaxies: the critical importance of star formation histories
• The H alpha Galaxy Survey. VIII. Close companions and interactions, and the definition of starbursts
• Hubble Space Telescope Grism Spectroscopy of Extreme Starbursts Across Cosmic Time: The Role of Dwarf Galaxies in the Star Formation History of the Universe
• The MaGICC volume: reproducing statistical properties of high redshift galaxies
• The evolution of the star forming sequence in hierarchical galaxy formation models
• Star formation in the CDFS: observations confront simulations
• Arp220: extinction and merger-induced star formation
• Parametrising Star Formation Histories
• The main sequence of star-forming galaxies at z~0.6: reinstating major mergers
• Characterizing simulated galaxy stellar mass histories

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