Star Formation and Feedback in Smoothed Particle Hydrodynamic Simulations--I. Isolated Galaxies

Abstract

We present an analysis of star formation and feedback recipes appropriate for galactic smoothed particle hydrodynamics simulations. Using an isolated Milky Way-like galaxy, we constrain these recipes based on well-established observational results. Our star formation recipe is based on that of Katz (1992) with the additional inclusion of physically motivated supernova feedback recipes. We propose a new feedback recipe in which type II supernovae are modelled using an analytical treatment of blastwaves. With this feedback mechanism and a tuning of other star formation parameters, the star formation in our isolated Milky Way-like galaxy is constant and follows the slope and normalisation of the observed Schmidt law. In addition, we reproduce the low density cutoff and filamentary structure of star formation observed in disk galaxies. Our final recipe will enable better comparison of cosmological N-body simulations with observations.

18 pages, 22 figures, accepted to MNRAS, full resolution figures, more data, and movies at http://hpcc.astro.washington.edu/starformation

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• Galactic angular momentum in cosmological zoom-in simulations. I. Disk and bulge components and the galaxy--halo connection
• The Relative Role of Galaxy Mergers and Cosmic Flows in Feeding Black Holes
• Black hole growth and AGN feedback under clumpy accretion
• NIHAO XVI: The properties and evolution of kinematically selected discs, bulges and stellar haloes
• NIHAO XXII: Introducing black hole formation, accretion and feedback into the NIHAO simulation suite
• A thermal-kinetic subgrid model for supernova feedback in simulations of galaxy formation
• The Main Sequence and the Fundamental Metallicity Relation in MaGICC Galaxies: Evolution and Scatter
• The edge of galaxy formation II: evolution of Milky Way satellite analogues after infall
• Fountains and storms: The role of AGN and mergers in disrupting the cool-core in the RomulusC simulation
• A unified model for age-velocity dispersion relations in Local Group galaxies: Disentangling ISM turbulence and latent dynamical heating
• Modeling for Stellar Feedback in Galaxy Formation Simulations
• The Effects of Ram-pressure Stripping and Supernova Winds on the Tidal Stirring of Disky Dwarfs: Enhanced Transformation into Dwarf Spheroidals
• Origin of the Metallicity Distribution in the Thick Disc
• Brightest Cluster Galaxies in Cosmological Simulations with Adaptive Mesh Refinement: Successes and Failures
• Numerical simulations of dwarf galaxy merger trees
• AGN Feedback models: Correlations with star formation and observational implications of time evolution
• Numerical Simulations of Bubble-Induced Star Formation in Dwarf Irregular Galaxies with a Novel Stellar Feedback Scheme
• The impact of early massive mergers on the chemical evolution of Milky Way-like galaxies: insights from NIHAO-UHD simulations
• Clumpy high-z galaxies as a testbed for feedback-regulated galaxy formation
• GRASIL-3D: an Implemention of Dust Effects in the SEDs of Simulated Galaxies
• Dark MaGICC: the effect of Dark Energy on galaxy formation. Cosmology does matter
• Not So Heavy Metals: Black Hole Feedback Enriches The Circumgalactic Medium
• The effect of non-equilibrium metal cooling on the interstellar medium
• How to bend galaxy disc profiles: the role of halo spin
• The stellar metallicity distribution of disc galaxies and bulges in cosmological simulations
• Galactic outflow and diffuse gas properties at z>=1 using different baryonic feedback models
• Effects of Inclination on Measuring Velocity Dispersion and Implications for Black Holes
• Reproducing cosmic evolution of galaxy population from $z=4$ to $0$
• The Formation of Compact Elliptical Galaxies in The Vicinity of A Massive Galaxy: The Role of Ram-pressure Confinement
• Internal Alignments of Red Versus Blue Discs in Dark Matter Halos
• An observational test for star formation prescriptions in cosmological hydrodynamical simulations
• The different baryonic Tully-Fisher relations at low masses
• A Kiloparsec-Scale Nuclear Stellar Disk in the Milky Way as a Possible Explanation of the High Velocity Peaks in the Galactic Bulge
• Emission from the circumgalactic medium: from cosmological zoom-in simulations to multiwavelength observables
• Delayed star formation in high-redshift stream-fed galaxies
• Formation and settling of a disc galaxy during the last 8 billion years in a cosmological simulation
• Rapid Filamentary Accretion as the Origin of Extended Thin Discs
• Massive central galaxies of galaxy groups in the Romulus simulations: an overview of galaxy properties at z=0
• Osaka Feedback Model II: Modeling Supernova Feedback Based on High-Resolution Simulations
• Formation of the first galaxies in the aftermath of the first supernovae
• CGM properties in VELA and NIHAO simulations; the OVI ionization mechanism: dependence on redshift, halo mass and radius
• MaGICC-WDM: the effects of warm dark matter in hydrodynamical simulations of disc galaxy formation
• Low-mass galaxy formation in cosmological AMR simulations: the effects of varying the sub-grid physics parameters
• Supernovae feedback propagation: the role of turbulence
• Beta Dips in the Gaia Era: Simulation Predictions of the Galactic Velocity Anisotropy Parameter for Stellar Halos
• Formation, disruption and energy output of Population III X-ray binaries
• What's in a name? Quantifying the interplay between the Definition, Orientation, and Shape of Ultra-diffuse Galaxies Using the Romulus Simulations
• Stars behind bars II: A cosmological formation scenario for the Milky Way's central stellar structure
• Reliability and limitations of inferring birth radii in the Milky Way disk
• Barred galaxies in cosmological zoom-in simulations: the importance of feedback
• Sowing black hole seeds: Direct collapse black hole formation with realistic Lyman-Werner radiation in cosmological simulations
• Super-critical accretion of medium-weight seed black holes in gaseous proto-galactic nuclei
• Simulating the H2 content of high-redshift galaxies
• How much metals did the first stars provide to the ultra-faint dwarfs?
• Uncertainties in supernova input rates drive qualitative differences in simulations of galaxy evolution
• How do different spiral arm models impact the ISM and GMC population?
• The response of dark matter haloes to elliptical galaxy formation: a new test for quenching scenarios
• Bar resilience to flybys in a cosmological framework
• Towards a self-consistent numerical model of late-type galaxies: Calibrating the effects of sub-grid physics on galactic models
• A New Model For Including Galactic Winds in Simulations of Galaxy Formation I: Introducing the Physically Evolved Winds (PhEW) Model
• NIHAO III: The constant disc gas mass conspiracy
• Constraints on the Shape of the Milky Way Dark Matter Halo from Jeans Equations Applied to SDSS Data
• Molecular cloud regulated star formation in galaxies
• Super massive black holes in star forming gaseous circumnuclear discs
• A semi-analytic model of the turbulent multi-phase interstellar medium
• Kinematic Evolution of Simulated Star-Forming Galaxies
• Dissecting Galaxy Formation: II. Comparing Substructure in Pure Dark Matter and Baryonic Models
• The Cosmic Baryon Partition between the IGM and CGM in the SIMBA Simulations
• Negative and Positive Feedback from a Supernova Remnant with SHREC: A detailed Study of the Shocked Gas in IC443
• Orbital support and evolution of flat profiles of bars (shoulders)
• NIHAO XXIV: Rotation or pressure supported systems? Simulated Ultra Diffuse Galaxies show a broad distribution in their stellar kinematics
• Survival of molecular gas in a stellar feedback-driven outflow witnessed with the MUSE TIMER project and ALMA
• The Cold Gas Content of Bulgeless Dwarf Galaxies
• Properties of thick discs formed in clumpy galaxies
• Star Formation and Feedback in Smoothed Particle Hydrodynamic Simulations II: Resolution Effects
• Probing Feedback via IGM tomography and Ly$\alpha$ forest with Subaru PFS, TMT/ELT, and JWST
• Can gravitational infall energy lead to the observed velocity dispersion in DLAs?
• The role of AGN feedback on the evolution of dwarf galaxies from cosmological simulations: SMBHs suppress star formation in low-mass galaxies
• GARROTXA Cosmological Simulations of Milky Way-sized Galaxies: General Properties, Hot Gas Distribution, and Missing Baryons
• Diffuse coronae in cosmological simulations of Milky Way-sized galaxies
• How to bend galaxy disc profiles II: stars surfing the bar in Type-III discs
• The Halo Shape and Evolution of Polar Disc Galaxies
• High resolution modeling of [CII], [CI], [OIII] and CO line emission from the ISM and CGM of a star forming galaxy at z ~ 6.5
• The Dawn of Disk Formation in a Milky Way-sized Galaxy Halo: Thin Stellar Disks at $z>4$
• Cosmic evolution of dust in galaxies: Methods and preliminary results
• A minor merger scenario for the ultraluminous X-ray source ESO 243-49 HLX-1
• Galaxy Outflows Without Supernovae
• Constraining the Tail-End of Reionization Using Lyman-$\alpha$ Transmission Spikes
• Cosmological simulations of Milky Way-sized galaxies
• A first estimate of the Milky Way dark matter halo spin
• Panspermia in a Milky Way-like Galaxy
• The Impact of Cosmic Rays on the Kinematics of the Circumgalactic Medium
• Young stars as tracers of a barred-spiral Milky Way
• A hidden population of massive black holes in simulated dwarf galaxies
• Comparing the Properties of GMCs in M33 from Simulations and Observations
• Chemical enrichment of stars due to accretion from ISM during the Galaxy's assembly
• The degeneracy between star-formation parameters in dwarf galaxy simulations and the Mstar-Mhalo relation
• The SATIN project I: Turbulent multi-phase ISM in Milky Way simulations with SNe feedback from stellar clusters
• Large-eddy simulations of isolated disc galaxies with thermal and turbulent feedback
• The complementary roles of feedback and mergers in building the gaseous halo and the X-ray corona of Milky Way-sized galaxies
• Simulations of isolated dwarf galaxies formed in dark matter halos with different mass assembly histories
• Stellar and Weak Lensing Profiles of Massive Galaxies in the Hyper-Suprime Cam Survey and in Hydrodynamic Simulations
• The global and radial stellar mass assembly of Milky Way-sized galaxies
• The H alpha Galaxy Survey V. The star formation history of late-type galaxies
• Age dissection of the vertical breathing motions in Gaia DR2: evidence for spiral driving
• Comparing galactic satellite properties in hydrodynamical and Nbody simulations
• Around The Way: Testing $\Lambda$CDM with Milky Way Stellar Stream Constraints
• Ultraviolet Signatures of the Multiphase Intracluster and Circumgalactic Media in the RomulusC Simulation
• The imprint of clump formation at high redshift. II. The chemistry of the bulge
• Evaluating Galaxy Dynamical Masses From Kinematics and Jeans Equilibrium in Simulations
• Halo orbits in cosmological disk galaxies: tracers of formation history
• Advanced Morphological Galaxy Classification: A Comparison of Real and Simulated Galaxies
• The small and the beautiful: How the star formation law affects galactic disk structure
• The history of stellar metallicity in a simulated disc galaxy
• Galaxy Formation with Local Photoionization Feedback -II. Effect of X-Ray Emission from Binaries and Hot Gas
• The AGORA High-resolution Galaxy Simulations Comparison Project. VI. Similarities and Differences in the Circumgalactic Medium
• H2 chemistry in galaxy simulations: an improved supernova feedback model
• A Moving Mesh Hydrodynamic Solver for ChaNGa
• Effects of feedback on galaxies in the VELA simulations: elongation, clumps and compaction
• Real and counterfeit cores: how feedback expands halos and disrupts tracers of inner gravitational potential in dwarf galaxies
• Galactic winds - How to launch galactic outflows in typical Lyman-break galaxies
• SImulator of GAlaxy Millimetre/submillimetre Emission (SIGAME): CO emission from massive z=2 main-sequence galaxies
• Bending waves excited by irregular gas inflow along warps
• The baryon cycle of Seven Dwarfs with superbubble feedback
• Local photoionization feedback effects on galaxies
• GMC Evolution in a Barred Spiral Galaxy with Star Formation and Thermal Feedback
• MaNGA galaxy properties -- II. A detailed comparison of observed and simulated spiral galaxy scaling relations
• NIHAO XXVI: Nature versus nurture, the Star Formation Main Sequence and the origin of its scatter
• Clumpy galaxies in cosmological simulations: The effect of ISM model
• One-Two Quench: A Double Minor Merger Scenario
• The effect of gravitational tides on dwarf spheroidal galaxies
• Time Dependent Radiation Hydrodynamics on a Moving Mesh
• The edge of galaxy formation III: The effects of warm dark matter on Milky Way satellites and field dwarfs
• Calibration of a star formation and feedback model for cosmological simulations with Enzo
• Momentum Injection by Clustered Supernovae: Testing Subgrid Feedback Prescriptions
• Simplified galaxy formation with mesh-less hydrodynamics
• Radiation pressure in galactic disks: stability, turbulence, and winds in the single-scattering limit
• Multiple regimes and coalescence timescales for massive black hole pairs ; the critical role of galaxy formation physics
• The diversity of spiral galaxies explained
• Stellar cluster formation in a Milky Way-sized galaxy at z>4 -- I. The proto-globular cluster population and the imposter amongst us
• Evolution of stellar-gaseous disks in cosmological haloes
• Explaining the chemical trajectories of accreted and in-situ halo stars of the Milky Way
• Testing Feedback from Star Clusters in Simulations of the Milky Way Formation
• Momentum and energy injection by a supernova remnant into an inhomogeneous medium
• Influence of baryonic physics in galaxy simulations: a semi-analytic treatment of the molecular component
• Testable predictions of outside-in age gradients in dwarf galaxies of all types
• Chemo-dynamical simulations of dwarf galaxy evolution
• Generation of gravitational waves and tidal disruptions in clumpy galaxies
• The relative efficiencies of bars and clumps in driving disc stars to retrograde motion
• Particle tagging and its implications for stellar population dynamics
• Star Formation and Gas Phase History of the Cosmic Web
• The luminosity function of diverse satellite galaxy systems
• Predicted Stellar Kinematics of a Kiloparsec-Scale Nuclear Disc (or Ring) in the Milky Way
• Heating and enriching the intracluster medium
• Differences in star formation activity between tidally triggered and isolated bars: a case study of NGC 4303 and NGC 3627
• Analytic and numerical realisations of a disk galaxy
• A Unified Exploration of the Chronology of the Galaxy
• The Properties of Bound and Unbound Molecular Cloud Populations Formed in Galactic Disc Simulations
• The temperature of hot gas in galaxies and clusters: baryons dancing to the tune of dark matter
• Little Red Dots as Direct-collapse Black Hole Nurseries
• Constraining the subgrid physics in simulations of isolated dwarf galaxies
• Mechanical feedback from stellar winds with an application to galaxy formation at high redshift
• Progenitor-mass-dependent yields amplify intrinsic scatter in dwarf-galaxy elemental abundance ratios
• Storm fronts over galaxy discs: Models of how waves generate extraplanar gas and its anomalous kinematics
• Metallicity profiles of Ultra Diffuse Galaxies in NIHAO simulations
• Connecting stellar and galactic scales: Energetic feedback from stellar wind bubbles to supernova remnants
• A high fidelity Milky Way simulation with Kraken, Gaia-Enceladus, and Sequoia analogues: clues to their accretion histories
• Self-Interacting Dark Matter and the Delay of Super-Massive Black Hole Growth
• Recent progress in simulating galaxy formation from the largest to the smallest scales
• CLUES about M33: the reversed radial stellar age gradient in the outskirts of Triangulum galaxy
• The Role of Quasar Radiative Feedback on Galaxy Formation during Cosmic Reionization
• Numerical simulations of bar formation in the Local Group
• Angular momentum evolution of bulge stars in disc galaxies in NIHAO
• Critical Metallicity of Cool Supergiant Formation. I. Effects on Stellar Mass Loss and Feedback
• Origin and Evolution of Structure and Nucleosynthesis for Galaxies in the Local Group
• Consequences of cosmic microwave background-regulated star formation
• Bursty Star Formation in Dwarfs is Sensitive to Numerical Choices in Supernova Feedback Models
• An Enhanced Massive Black Hole Occupation Fraction Predicted in Cluster Dwarf Galaxies
• The origin of type-I profiles in cluster lenticulars: An interplay between ram pressure stripping and tidally-induced spiral migration
• The Impact of Wind Scalings on Stellar Growth and the Baryon Cycle in Cosmological Simulations
• Milky Way-like galaxies: stellar population properties of dynamically defined disks, bulges and stellar halos
• The tilting rate of the Milky Way's disc
• Dynamic equilibrium sets atomic content of galaxies across cosmic time
• Drivers of disc tilting I: Correlations and possible drivers for Milky Way analogues
• Effective viscosity from cloud-cloud collisions in three-dimensional global SPH simulations
• Origin of stellar prolate rotation in a cosmologically simulated faint dwarf galaxy
• Numerical dependencies of the galactic dynamo in isolated galaxies with SPH
• Implementing Dust Shielding as a Criteria for Star Formation
• On the Functional Form of the Universal Star Formation Law
• DLA kinematics and outflows from starburst galaxies
• Non-explosive pre-supernova feedback in the COLIBRE model of galaxy formation
• Haloes at the ragged edge: The importance of the splashback radius
• Bar-spiral interaction produces radial migration and star formation bursts
• Where Did the Outskirts Go? Outer Stellar Haloes as a Sensitive Probe of Supernova Feedback
• The Radial Distribution of Mono-Metallicity Populations in the Galactic Disk as Evidence for Two-Phase Disk Formation
• The Pressure of the Star Forming ISM in Cosmological Simulations
• NIHAO XXVIII: Collateral effects of AGN on dark matter concentration and stellar kinematics
• The life cycle of giant molecular clouds in simulated Milky Way-mass galaxies
• High accuracy power spectra including baryonic physics in dynamical Dark Energy models
• Disc-Halo Interactions in ΛCDM
• HELLO project: High-$z$ Evolution of Large and Luminous Objects
• Predicted Trends in Milky Way Bulge Proper Motion Rotation Curves: future Prospects for HST and LSST
• Predictions for Detecting a Turndown in the Baryonic Tully Fisher Relation
• NIHAO XXVII: Crossing the green valley
• A MARVEL-ous study of how well galaxy shapes reflect Dark Matter halo shapes in Cold Dark Matter Simulations
• COLIBRE: calibrating subgrid feedback in cosmological simulations that include a cold gas phase
• How stars formed in warps settle into (and contaminate) thick discs
• Cloud angular momentum and effective viscosity in global SPH simulations with feedback
• Potential Impact of the Sagittarius Dwarf Galaxy on the Formation of Young O-rich Stars
• The Evolution of Magellanic-like Galaxy Pairs and The Production of Magellanic Stream Analogues in Simulations with Tides, Ram Pressure, and Stellar Feedback
• The galaxy counterpart of the high-metallicity and 16 kpc impact parameter DLA towards Q0918+1636 - a challenge to galaxy formation models?
• Using Artificial Intelligence and real galaxy images to constrain parameters in galaxy formation simulations
• NIHAO-RiNG: A Comparison of Simulated Disc Galaxies from GASOLINE and GIZMO
• Multi-scale simulations of black hole accretion in barred galaxies: Self-gravitating disk models
• Diversity of dwarf galaxy IR-submm emission patterns: CLUES from hydrodynamical simulations
• Does slow and steady win the race? Investigating feedback processes in giant molecular clouds
• Survivors and Zombies: The Quenching and Disruption of Satellites around Milky Way Analogs
• Quenching vs. Quiescence: forming realistic massive ellipticals with a simple starvation model
• Constraining gas metal mixing strength in simulations using observations of the Milky Way's disc
• Refueled and shielded - The early evolution of Tidal Dwarf Galaxies
• A New Multi-Scale Structure Finding Algorithm to Identify Cosmological Structure
• Testing the Momentum-driven Supernova Feedback Paradigm in M31
• Growth and Feedback from the First Black Holes
• Spectral reconstruction for radiation hydrodynamic simulations of galaxy evolution
• Galaxy mass profiles with convolutional neural networks
• Merging Black Holes in Dwarf Galaxies: Calculating Binary Black Hole Coalescence Timescales from Simulations for LISA Detection
• Intermediate Mass Ratio Inspirals in Milky Way Galaxies
• QSO MUSEUM III: the circumgalactic medium in Ly$\alpha$ emission around 120 $z\sim 3$ quasars covering the SDSS parameter space. Witnessing the instantaneous AGN feedback on halo scales
• The Chemical and Dynamical Evolution of Isolated Dwarf Galaxies
• A theoretical investigation of far-infrared fine structure lines at $z>6$ and of the origin of the [OIII]88/[CII]158 enhancement
• Cosmic wallflowers: the circumgalactic origins of isolated ultra-compact star clusters at $z>7$
• Dynamical disequilibrium in dwarf galaxies: rethinking gas dynamics, rotation curves, and dark matter inference
• Too small to succeed: the difficulty of sustaining star formation in low-mass haloes
• Quantitatively rating galaxy simulations against real observations with anomaly detection
• How Many Bursts Does it Take to Form a Core at the Center of a Galaxy?
• Bridging Simulations and Observations: New Insights into Galaxy Formation Simulations via Out-of-Distribution Detection and Bayesian Model Comparison
• NIHAO-LG: The uniqueness of Local Group dwarf galaxies
• A New Model For Including Galactic Winds in Simulations of Galaxy Formation II: Implementation of PhEW in Cosmological Simulations
• MAUVE: An Ultraviolet Astrophysics Probe Mission Concept
• The chemical and spatial variations of the bulge's velocity ellipsoids
• The Lowest Metallicity Stars in the LMC: Clues from MaGICC Simulations
• The Role of Mass and Environment on Satellite distributions around Milky Way analogs in the Romulus25 simulation
• ARCHITECTS I: Impact of subgrid physics on the simulated properties of the circumgalactic medium
• The Formation of Dwarf Galaxy Disks
• High precision spectra at large redshift for dynamical DE cosmologies
• Bar Properties and Star-by-Star Bar Membership via Action Conservation
• Momentum deposition of supernovae with cosmic rays
• Size-scaling of clump instabilities in turbulent, feedback regulated disks
• Turning Points in the Age-Metallicity Relations -- Created by Late Satellite Infall and Enhanced by Radial Migration
• Forged by Feedback: Stellar Properties of Brightest Group Galaxies in Cosmological Simulations
• A probabilistic deep learning model to distinguish cusps and cores in dwarf galaxies
• The importance of the way in which supernova energy is distributed around young stellar populations in simulations of galaxies
• Dust and gas modelling in radiative transfer simulations of disc-dominated galaxies with RADMC-3D
• The Supernova-ISM/Star formation Interplay
• Supernovae and photoionizing feedback in spiral arm molecular clouds
• Starburst galaxies in the Hydra I cluster
• Beyond single tracers: CNN-based inference of galaxy mass profiles from combined gas and stellar kinematics
• The chemodynamical memory of a major merger in a NIHAO-UHD Milky Way analogue -- I. A golden thread through time and space
• The Impact of Star Formation Histories on the Inner Dark Matter Density Slopes of Galaxies
• Modeling supernova feedback in galaxy formation simulations with energy-conserving momentum injection
• Phase spirals induced by the gas warp
• A thick-disk galaxy model and simulations of equal-mass galaxy pair collisions