The First Stars
arXiv:astro-ph/0311019 · doi:10.1146/annurev.astro.42.053102.134034
Abstract
We review recent theoretical results on the formation of the first stars in the universe, and emphasize related open questions. In particular, we discuss the initial conditions for Population III star formation, as given by variants of the cold dark matter cosmology. Numerical simulations have investigated the collapse and the fragmentation of metal-free gas, showing that the first stars were predominantly very massive. The exact determination of the stellar masses, and the precise form of the primordial initial mass function, is still hampered by our limited understanding of the accretion physics and the protostellar feedback effects. We address the importance of heavy elements in bringing about the transition from an early star formation mode dominated by massive stars, to the familiar mode dominated by low mass stars, at later times. We show how complementary observations, both at high redshifts and in our local cosmic neighborhood, can be utilized to probe the first epoch of star formation.
38 pages, 10 figures, draft version for 2004 Annual Reviews of Astronomy and Astrophysics, high-resolution version available at http://cfa-www.harvard.edu/~vbromm/
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- Constraining Dark Matter properties with the first generation of stars
- Blocking metal accretion onto population III stars by stellar wind
- Search for blue compact dwarf galaxies during quiescence II: metallicities of gas and stars, ages, and star-formation rates
- Supermassive Black Holes in the Early Universe
- Population III Star Clusters in the Reionized Universe
- Massive Black Hole Science with eLISA
- Pair Correlations and Merger Bias
- Formation of Galactic Systems in Light of the Magnesium Abundance in Field Stars: The Thick Disk
- Nuclear processes in Astrophysics: Recent progress
- Growth of Supermassive Black Hole Seeds in ETG Star-Forming Progenitors: Multiple Merging of Stellar Compact Remnants via Gaseous Dynamical Friction and Gravitational Wave Emission
- Astrophysical S factor for the radiative capture 12N(p,gamma)13O determined from the 14N(12N,13O)13C proton transfer reaction
- The HI content of extremely metal-deficient blue compact dwarf galaxies
- Ultrafaint Dwarfs - Star Formation and Chemical Evolution in the Smallest Galaxies
- Gamma-ray bursts and Population III stars
- Modelling the cosmological Lyman-Werner background radiation field in the Early Universe
- Gravitational-wave captures by intermediate-mass black holes in galactic nuclei
- Chemical enrichment of stars due to accretion from ISM during the Galaxy's assembly
- Molecular Chemistry for Dark Matter II: Recombination, Molecule Formation, and Halo Mass Function in Atomic Dark Matter
- Ultraluminous X-ray sources: three exciting years
- Studying Cosmic Dawn using redshifted HI 21-cm signal: A brief review
- Impact of an accurate modeling of primordial chemistry in high resolution studies
- Dark matter powered stars: Constraints from the extragalactic background light
- The implications of dust for high-redshift protogalaxies and the formation of binary disks
- Intermediate-mass Black Holes on the Run from Young Star Clusters
- Gravitational stability and fragmentation condition for discs around accreting supermassive stars
- Mixing of Primordial Gas in Lyman Break Galaxies
- The role of the H adiabatic index in the formation of the first stars
- Gravitational wave probes of particle dark matter: a review
- Hot Cores : Probes of High-Redshift Galaxies
- Fragmentation in Dusty Low-Metallicity Star Forming Halos
- The Pristine survey -- XV. A CFHT ESPaDOnS view on the Milky Way halo and disc populations
- Growth of Early Supermassive Black Holes and the High-Redshift Eddington Ratio Distribution
- Multicomponent multiscatter capture of Dark Matter
- Where can we really find the First Stars' Remnants today?
- The clustering properties of the first galaxies
- Potential signature of Population III pair-instability supernova ejecta in the BLR gas of the most distant quasar at z = 7.54
- CEMP stars: possible hosts to carbon planets in the early universe
- Cold accretion in early galaxy formation and its Lyman-alpha signatures
- Cosmic evolution of metal densities: the enrichment of the Inter-Galactic Medium
- Mining S-PLUS for Metal-Poor Stars in the Milky Way
- Properties and merger signatures of galaxies hosting LISA coalescing massive black hole binaries
- Black Holes in our Galactic Halo: Compatibility with FGST and PAMELA Data and Constraints on the First Stars
- Origin of metals in old Milky Way halo stars based on GALAH and Gaia
- Probing the Pre-Reionization Epoch with Molecular Hydrogen Intensity Mapping
- Impact of magnetic fields on Population III star formation
- Probing Intermediate Mass Black Holes in M87 through Multi-Wavelength Gravitational Wave Observations
- Extremely-Metal Poor Stars in the Milky Way: A Second Generation Formed after Reionization
- Evidence of Pop~III stars' chemical signature in neutral gas at z~6. A study based on the E-XQR-30 spectroscopic sample
- Photometric Properties of the Most Massive High-Redshift Galaxies
- 21cmFirstCLASS I. Cosmological tool for CDM and beyond
- SIEGE III: The formation of dense stellar clusters in sub-parsec resolution cosmological simulations with individual star feedback
- The First Stars: formation under cosmic ray feedback
- Enhanced direct collapse due to Lyman alpha feedback
- Inferring the velocity of early massive stars from the abundances of extremely metal-poor stars
- Cosmological Impact of Population III Binaries
- Dark Stars: A New Study of the FIrst Stars in the Universe
- On the operation of the chemothermal instability in primordial star-forming clouds
- An upper limit on the sulphur abundance in HE 1327-2326
- An Observational Test for the Anthropic Origin of the Cosmological Constant
- The G-dwarf problem in the Galaxy
- Candidate X-ray-Emitting OB Stars in the MYStIX Massive Star-Forming Regions
- Sources for Metals in the Intergalactic Medium
- The Age-Metallicity Relation in the Thin Disk of the Galaxy
- Can Population III stars be major origins of both merging binary black holes and extremely metal poor stars?
- Rapid formation of a very massive star >50000 and subsequently an IMBH from runaway collisions. Direct N-body and Monte Carlo simulations of dense star clusters
- Intermediate-mass black holes in dwarf galaxies: the case of Holmberg II
- Implications of primordial black holes on the first stars and the origin of the super--massive black holes
- The central engine of the highest redshift blazar
- Cosmic Chemical Evolution with an Early Population of Intermediate Mass Stars
- Multiscale mass transport in z~6 galactic discs: fueling black holes
- Determination of astrophysical 12N(p,g)13O reaction rate from the 2H(12N, 13O)n reaction and its astrophysical implications
- Constraining the cosmic merger history of intermediate-mass black holes with gravitational wave detectors
- Metal Pollution of Low-Mass Population III Stars through Accretion of Interstellar Objects like `Oumuamua
- First stars as a possible origin for the helium-rich population in omega Centauri
- The Stars of the HETDEX Survey. I. Radial Velocities and Metal-Poor Stars from Low-Resolution Stellar Spectra
- Feedback from Multiple Supernova Explosions inside a Wind-Blown Bubble
- A chemical signature from fast-rotating low-metallicity massive stars: ROA 276 in omega Centauri
- The Cosmic Evolution of Fast Radio Bursts Inferred from the CHIME/FRB Baseband Catalog 1
- Effect of Population III Multiplicity on Dark Star Formation
- Search for Extremely Metal-Poor Stars with GEMINI-N/GRACES I. Chemical-Abundance Analysis
- Formation of Compact Stellar Clusters by High-Redshift Galaxy Outflows II: Effect of Turbulence and Metal-Line Cooling
- The Halo Occupation Distribution of Black Holes: Dependence on Mass
- The First Billion Years in Seconds: An Effective Model for the 21-cm Signal with Population III Stars
- The effect of diffuse background on the spatially-resolved Schmidt relation in nearby spiral galaxies
- The effect of dark matter resolution on the collapse of baryons in high redshift numerical simulations
- GRBs and fundamental physics
- Footprints of population III stars in the gravitational-wave background
- Calibrating the binary black hole population in nuclear star clusters through tidal disruption events
- Impact of H-driven star formation and stellar feedback from low-enrichment environments on the formation of spiral galaxies
- Constraining HeII Reionization Detection Uncertainties via Fast Radio Bursts
- Hunting intermediate-mass black holes with LISA binary radial velocity measurements
- Impact of Rotation on Neutrino Emission and Relic Neutrino Background from Population III Stars
- Gas Accretion and Star Formation Rates
- Black Hole Formation and Explosion from Rapidly Rotating Very Massive Stars
- The X-ray Properties of the Cometary Blue Compact Dwarf galaxies Mrk 59 and Mrk 71
- Intermediate-mass black hole binary parameter estimation with next-generation ground-based detector networks
- The first spectral line surveys searching for signals from the Dark Ages
- Multiscatter capture of superheavy dark matter by Pop. III stars
- Supermassive black hole seeds from sub-keV dark matter
- The role of 3-body H formation in the fragmentation of primordial gas
- Dust Production Factories in the Early Universe: Formation of Carbon Grains in Red-supergiant Winds of Very Massive Population III Stars
- Observational nuclear astrophysics: neutron-capture element abundances in old, metal-poor stars
- Dark Stars and Boosted Dark Matter Annihilation Rates
- The S-PLUS Ultra-Short Survey: first data release
- Compact Objects in close orbits as Gravitational Wave Sources: Formation Scenarios and Properties
- Connecting the Cosmic Star Formation Rate with the Local Star Formation
- The inhomogenous reionization of the inter-galactic medium by metal-poor globular clusters
- Direct Collapse to Supermassive Black Hole Seeds: Comparing the AMR and SPH Approaches
- The EDGES measurement disfavors an excess radio background during the cosmic dawn
- State-resolved rotational cross sections and thermal rate coefficients for ortho-/para-H2+HD at low temperatures and HD+HD elastic scattering
- Effects of feedback-free starburst galaxies on the 21-cm signal and reionization history
- Formation of metal-free binaries: Impact of H line cooling and CIE cooling
- Very metal-poor stars in the solar vicinity: age determination
- The early phases of Milky Way's chemical evolution
- The Science Case for PILOT II: the Distant Universe
- Early formation of supermassive black holes from the collapse of strongly self-interacting dark matter
- Reassessing Dust's Role in Forming the CMB
- Applications of Stellar Population Synthesis in the Distant Universe
- Do fragmentation and accretion affect the stellar Initial Mass Function?
- Progenitors of Long-Duration Gamma-ray Bursts
- J1342+0928 Supports the Timeline in the R_h=ct Cosmology
- Astrophysical Explosions: From Solar Flares to Cosmic Gamma-ray Bursts
- On the effects of rotation in primordial star-forming clouds
- A search for Population III galaxies in CLASH. I. Singly-imaged candidates at high redshift
- Downsizing of Star-Forming Galaxies by Gravitational Processes
- Detectability of Supermassive Dark Stars with the Roman Space Telescope
- HD molecule and search for early structure-formation signatures in the Universe
- Does the chemothermal instability have any role in the fragmentation of primordial gas
- Chemodynamical Properties and Ages of Metal-Poor Stars in S-PLUS
- An Empirical Calibration of the Helium Abundance in HII Regions based in Literature and CALIFA Survey data
- Contribution of the first galaxies to the cosmic far-infrared/sub-millimeter background - I. Mean background level
- Menus for Feeding Black Holes
- Resistive Heating Induced by Streaming Cosmic Rays Around a Galaxy in the Early Universe
- Cosmological X-ray Scattering from Intergalactic Dust
- Stellar Evolution at Low Metallicity
- Analytic Approximations for the Velocity Suppression of Dark Matter Capture
- The formation of the first galaxies and the transition to low-mass star formation
- Joint 21-cm and CMB Forecasts for Constraining Self-Interacting Massive Neutrinos
- Coronal Properties of Low-mass Population III Stars and the Radiative Feedback in the Early Universe
- Open questions in the study of population III star formation
- The Masses of Supernova Remnant Progenitors in M33
- A chemodynamical analysis of bright metal-poor stars from the HESP-GOMPA survey -- Indications of a non-prevailing site for light r-process elements
- The Low-Mass Stellar Initial Mass Function in Nearby Ultrafaint Dwarf Galaxies
- Quasi-star jets as unidentified gamma-ray sources
- Formation of the First Galaxies: Theory and Simulations
- Synthetic Spectra of Pair-Instability Supernovae in 3D
- Understanding Galaxy Formation and Evolution
- Mapping the Distant and Metal-Poor Milky Way with SDSS-V
- Metal Enrichment and Reionization Constraints on Early Star Formation
- First Stars. I. Evolution without mass loss
- The effects of convection criteria on the evolution of population III stars and the detectability of their supernovae
- Probing Long-Range Forces Between Neutrinos with Cosmic Structures
- Geoastronomy: Rocky planets as the Lavosier-Lomonosov Bridge from the non-living to the living world
- Atomic Modeling of Photoionization Fronts in Nitrogen Gas
- First Star Survivors as Metal-Rich Halo Stars that Experienced Supernova Explosions in Binary Systems
- Holography, large scale structure, supermassive black holes, and minimum stellar mass
- Probing the physics and history of cosmic reionization with the Sunyaev-Zel'dovich Effect
- Simulating the collapse of rotating primordial gas clouds to study the survival possibility of Pop III protostars
- Spherically symmetric NLTE model atmospheres of hot hydrogen-helium first stars
- A Pop III generated dust screen at z~16
- The impact of wind mass loss on nucleosynthesis and yields of very massive stars at low metallicity
- The influence of baryons on low-mass haloes
- Impact of accretion-induced chemically homogeneous evolution on stellar and compact binary populations
- Chemical Evolution of the Juvenile Universe
- Redshift Horizon for Detecting the First Galaxies in Far-Infared Surveys
- Cosmic microwave background constraints on a decaying cosmological term related to the thermal evolution
- Central Engine and Spectral Energy Distribution Properties of High Redshift Gamma Ray Blazars
- Reconstructing the star formation rate for compact binary populations with the Einstein telescope
- Supernovae at the cosmic dawn
- Metal Enrichment of the Intergalactic Medium and Production of Massive Black Holes
- Cosmic Bandits: Exploration versus Exploitation in CMB B-Mode Experiments
- Hierarchical Object Formation in the Peculiar Velocity Field
- Fluorine abundances in CEMP stars at the lowest metallicity: Hints on the nature of the first stars
- Understanding Stellar Mass-Metallicity and Size Relations in Simulated Ultra-Faint Dwarf Galaxies
- Spatial Correlation of Massive Black Hole Mergers: Probing the Formation Mechanism and Reionization
- Searching for Pop III stars and galaxies at high redshift
- Zero Metallicity with Zero CPU Hours: Masses of the First Stars on the Laptop
- Detection for Intermediate-mass Binary Black Holes in Population III Star Clusters with TianQin
- Angular momentum distribution during the collapse of primordial star-forming clouds
- The Halo Mass Function Redshift Dependence
- Impact of Population III stars on the astrophysical gravitational-wave background
- CHEERS: Future perspectives for abundance measurements in clusters with XMM-Newton
- Discovery of three new near-pristine absorption clouds at -4.4
- Complexity in small-scale dwarf spheroidal galaxies
- Understanding the IMF
- Detectability of Population III stellar remnants as X-ray binaries from tidal captures in the local Universe
- Formation and Evolution of Supermassive Black Holes
- The Anomalous 21-cm Absorption at High Redshifts
- Large-scale variability in macroturbulence driven by pulsations in the rapidly rotating massive star Zeta Oph from high-cadence ESPRESSO spectroscopy and TESS photometry
- Estimating the evolution of gas in the Fornax dwarf spheroidal galaxy from its star formation history: an illustrative example
- Star Formation for Predictive Primordial Galaxy Formation
- First Stars. II. Evolution with mass loss
- Supermassive Dark Stars and their remnants as a possible solution to three recent cosmic dawn puzzles
- Implications of the cosmic infrared background excess for the cosmic star formation
- HE0144-4657: A Carbon-Enhanced Ultra Metal-Poor Star ([Fe/H] ~ -4.1) from the Helmi Stream Disrupted Dwarf Galaxy
- Observing the influence of growing black holes on the pre-reionization IGM
- Dark Stars: Dark Matter in the First Stars leads to a New Phase of Stellar Evolution
- Very Massive Close Binaries and the Puzzling Temporal Evolution of 14N in the Solar Neighbourhood
- Revealing the formation histories of the first stars with the cosmic near-infrared background
- The First Stars
- Dark-Matter-Powered Population III Evolution: Lifetimes, Rotation, and Quasi-Homogeneity in massive Stars
- Early Cosmic Chemical Evolution: Relating the Origin of a Diffuse Intergalactic Medium and the First Long-Lived Stars
- Merger rates of intermediate-mass black hole binaries in nuclear star clusters
- Radio Spectral Energy Distributions for Single Massive Star Winds with Free-Free and Synchrotron Emission
- The symphony of pulsations and binarity among massive stars using HERMES spectroscopy and TESS photometry
- Studying The Effect of Radiation Pressure on Evolution of a Population III Stellar Cluster
- Imprint of first stars era in the cosmic infrared backround fluctuations
- Direct N-body simulations of rotating and extremely massive Population III star clusters
- Off-center black hole seed formation? Implications for high and low redshift massive black holes
- Space Project for Astrophysical and Cosmological Exploration (SPACE), an ESA stand-alone mission and a possible contribution to the Origins Space Telescope
- LYRA II: Cosmological dwarf galaxy formation with inhomogeneous Population III enrichment
- Simulations of Early Galaxy Formation
- First Light: Switching on Stars at the Dawn of Time
- The Effect of Environment on Massive Star Formation