The star formation main sequence and stellar mass assembly of galaxies in the Illustris simulation
arXiv:1409.0009 · doi:10.1093/mnras/stu2713
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 (30)
- The EAGLE project: Simulating the evolution and assembly of galaxies and their environments
- Introducing the Illustris Project: Simulating the coevolution of dark and visible matter in the Universe
- Cold streams in early massive hot haloes as the main mode of galaxy formation
- UV Star Formation Rates in the Local Universe
- A Highly Consistent Framework for the Evolution of the Star-Forming "Main Sequence" from z~0-6
- Properties of galaxies reproduced by a hydrodynamic simulation
- Introducing the Illustris Project: the evolution of galaxy populations across cosmic time
- Formation of Massive Galaxies at High Redshift: Cold Streams, Clumpy Disks and Compact Spheroids
- A unified model for AGN feedback in cosmological simulations of structure formation
- 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
- On the frequency, intensity and duration of starburst episodes triggered by galaxy interactions and mergers
- On the Lack of Evolution in Galaxy Star Formation Efficiency
- Galaxy growth in the concordance CDM cosmology
- Halo Mass and Assembly History Exposed in the Faint Outskirts: the Stellar and Dark Matter Haloes of Illustris Galaxies
- SMA Imaging of CO(3-2) Line and 860 micron Continuum of Arp 220 : Tracing the Spatial Distribution of Luminosity
- 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?
- Understanding the Structural Scaling Relations of Early-Type Galaxies
- 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 evolution of the star forming sequence in hierarchical galaxy formation models
- Parametrising Star Formation Histories
- The main sequence of star-forming galaxies at z~0.6: reinstating major mergers
- Characterizing simulated galaxy stellar mass histories
Cited by in corpus (88)
- Simba: Cosmological Simulations with Black Hole Growth and Feedback
- The Herschel view of the dominant mode of galaxy growth from z=4 to the present day
- The Illustris simulation: the evolving population of black holes across cosmic time
- Constraining the properties of AGN host galaxies with Spectral Energy Distribution modeling
- Fast, Slow, Early, Late: Quenching Massive Galaxies at z~0.8
- Non-parametric Star Formation History Reconstruction with Gaussian Processes I: Counting Major Episodes of Star Formation
- MUFASA: Galaxy star formation, gas, and metal properties across cosmic time
- A New Census of the 0.2< z <3.0 Universe, Part II: The Star-Forming Sequence
- CEERS Key Paper V: A triality on the nature of HST-dark galaxies
- Atomic and molecular gas in IllustrisTNG galaxies at low redshift
- The Diversity and Variability of Star Formation Histories in Models of Galaxy Evolution
- X-rays across the galaxy population I: tracing the main sequence of star formation
- SDSS-IV MaNGA: Effects of Morphology in the global and local Star Formation Main Sequences
- When did Population III star formation end?
- The ALMA REBELS Survey: Specific Star-Formation Rates in the Reionization Era
- Identifying Galaxy Mergers in Observations and Simulations with Deep Learning
- The ALMaQUEST Survey: V. The non-universality of kpc-scale star formation relations and the factors that drive them
- Mini-quenching of galaxies by bursty star formation
- Exploring the physical properties of lensed star-forming clumps at
- Aperture-free star formation rate of SDSS star-forming galaxies
- The galaxy-halo connection of emission-line galaxies in IllustrisTNG
- The MOSDEF Survey: Metallicity Dependence of the PAH Emission at High Redshift and Implications for 24 micron-inferred IR Luminosities and Star Formation Rates at z~2
- The Relationship Between Star-formation Activity and Galaxy Structural Properties in CANDELS and a Semi-analytic Model
- The merger-starburst connection across cosmic times
- The assembly of dusty galaxies at : the build-up of stellar mass and its scaling relations with hints from early JWST data
- The early phases of galaxy clusters formation in IR: coupling hydrodynamical simulations with GRASIL3D
- Star Formation Stochasticity Measured from the Distribution of Burst Indicators
- Are star formation rates of galaxies bimodal?
- The high redshift SFR-M* relation is sensitive to the employed star formation rate and stellar mass indicators: Towards addressing the tension between observations and simulations
- Is there enough star formation in simulated protoclusters?
- An alternate approach to measure specific star formation rates at 2<z<7
- An evolving and mass dependent - relation for galaxies
- The Extreme Low-mass End of the Mass-Metallicity Relation at
- Blue Rest-Frame UV-Optical Colors in z~8 Galaxies from GREATS: Very Young Stellar Populations at ~650 Myr of Cosmic Time
- VINTERGATAN IV: Cosmic phases of star formation in Milky Way-like galaxies
- COSMOS2020: Manifold Learning to Estimate Physical Parameters in Large Galaxy Surveys
- Diffstar: A Fully Parametric Physical Model for Galaxy Assembly History
- The Escape Fraction of Ionizing Photons During the Epoch of Reionization: observability with the Square Kilometre Array
- A Virgo Environmental Survey Tracing Ionised Gas Emission (VESTIGE).XIV. The main sequence relation in a rich environment down to M_star ~ 10^6 Mo
- Stacked star formation rate profiles of bursty galaxies exhibit 'coherent' star formation
- The observability of galaxy merger signatures in nearby gas-rich spirals
- Star formation in galaxies hosting AGN: A flat trend of star-formation rate with X-ray luminosity of galaxies hosting AGN in the SCUBA-2 Cosmology Legacy Survey
- The interconnection between galaxy mergers, AGN activity and rapid quenching of star formation in simulated post-merger galaxies
- The miniJPAS survey: Identification and characterization of the emission line galaxies down to in the AEGIS field
- Surrogate modelling the Baryonic Universe II: on forward modelling the colours of individual and populations of galaxies
- Unraveling the interplay between SIDM and baryons in MW halos: defining where baryons dictate heat transfer
- Massive High-Redshift Quiescent Galaxies With JWST
- Cold and Hot gas distribution around the Milky-Way-M31 system in the HESTIA simulations
- Do galaxies die? Different views from simulations and observations in the Local Universe
- Formation and assembly history of stellar components in galaxies as a function of stellar and halo mass
- Discovery of a Dusty, Chemically Mature Companion to a z4 Starburst Galaxy in JWST ERS Data
- Dissecting Nearby Galaxies with piXedfit: II. Spatially Resolved Scaling Relations Among Stars, Dust, and Gas
- Variations in the slope of the resolved star-forming main sequence: a tool for constraining the mass of star-forming regions
- HI Global Scaling Relations in the WISE-WHISP Survey
- A hyper luminous starburst at z=4.72 magnified by a lensing galaxy pair at z=1.48
- Deep Extragalactic VIsible Legacy Survey (DEVILS): Evolution of the -M relation and implications for self-regulated star formation
- Trading oxygen for iron I: the [O/Fe] -- specific star formation rate relation of galaxies
- LEO-Py: Estimating likelihoods for correlated, censored, and uncertain data with given marginal distributions
- Centrally Concentrated H I Distribution Enhances Star Formation in Galaxies
- The miniJPAS survey: The galaxy populations in the most massive cluster in miniJPAS, mJPC2470-1771
- The Mass Growth and Stellar Ages of Galaxies: Observations versus Simulations
- Quenching, Mergers and Age Profiles for z=2 Galaxies in IllustrisTNG
- The parallelism between galaxy clusters and early-type galaxies: I. The light and mass profiles
- The hot gas mass fraction in halos. From Milky Way-like groups to massive clusters
- Star formation history and transition epoch of cluster galaxies based on the Horizon-AGN simulation
- The XXL survey. XLIX. Linking the members star formation histories to the cluster mass assembly in the z=1.98 galaxy cluster XLSSC 122
- Resolved star formation in TNG100 central and satellite galaxies
- Local Volume Late-Type Galaxies with an Extreme Ratio of -to- Star-Formation Rates
- A stochastic model to reproduce the star-formation history of individual galaxies in hydrodynamic simulations
- Improved Measurements of Galaxy Star Formation Stochasticity from the Intrinsic Scatter of Burst Indicators
- On the variation in stellar -enhancements of star-forming galaxies in the EAGLE simulation
- HELLO project: High- Evolution of Large and Luminous Objects
- Constraining the Active Galactic Nucleus and Starburst Properties of the IR-luminous Quasar Host Galaxy APM 08279+5255 at Redshift 4 with SOFIA
- Understanding the radio luminosity function of star-forming galaxies and its cosmological evolution
- Anatomy of galactic star formation history: Roles of different modes of gas accretion, feedback, and recycling
- Estimation of the Galaxy Quenching Rate in the Illustris Simulation
- Applying unsupervised learning to resolve evolutionary histories and explore the galaxy-halo connection in IllustrisTNG
- Cosmic Pathways for Compact Groups in the Milli-Millennium Simulation
- Probing the earliest phases in the formation of massive galaxies with simulated HST+JWST imaging data from Illustris
- DESI Emission-line Galaxies: Clustering Dependence on Stellar Mass and [OII] Luminosity
- The slope and scatter of the star forming main sequence at z~5 : reconciling observations with simulations
- The effects of star formation history in the SFR-M relation of HII galaxies
- Constraining galactic baryon cycle using the galaxy stellar-to-halo mass relations
- The Outskirt Stellar Mass of Low-Redshift Massive Galaxies is an Excellent Halo Mass Proxy in Illustris/IllustrisTNG Simulations
- Sub-Gyr variability around the SFMS and its contribution to the scatter
- Lack of influence of the environment in the earliest stages of massive galaxy formation
- The galaxy starburst/main-sequence bimodality over five decades in stellar mass at z ~ 3-6.5
- On the quenching of star formation in observed and simulated central galaxies: Evidence for the role of integrated AGN feedback