A Universal, Local Star Formation Law in Galactic Clouds, Nearby Galaxies, High-Redshift Disks, and Starbursts
arXiv:1109.4150 · doi:10.1088/0004-637X/745/1/69
Abstract
[abridged] While observations of Local Group galaxies show a very simple, local star formation law in which the star formation rate per unit area in each patch of a galaxy scales linearly with the molecular gas surface density, recent observations of both Milky Way molecular clouds and high redshift galaxies apparently show a more complicated relationship, in which regions of equal surface density can form stars at quite different rates. These data have been interpreted as implying either that different star formation laws apply in different circumstances, that the star formation law is sensitive to large-scale galaxy properties rather than local properties, or that there are high density thresholds for star formation. Here we collate resolved observations of Milky Way molecular clouds, kpc-scale observations of Local Group galaxies, and unresolved observations of both disk and starburst galaxies in the local universe and at high redshift. We show that all of these data are in fact consistent with a simple, local, volumetric star formation law. The apparent variations stem from the fact that the observed objects have a wide variety of 3D size scales and degrees of internal clumping, so even at fixed gas column density the regions being observed can have wildly varying volume densities. We provide a simple theoretical framework to remove this projection effect, and we show that all the data, from small Solar neighborhood clouds with masses ~10^3 Msun to sub-mm galaxies with masses ~10^11 Msun, fall on a single star formation law in which the SFR is simply ~1% of the molecular gas mass per local free-fall time. In contrast, proposed star formation laws in which the star formation timescale is set by the galactic rotation period or the SFR is linearly proportional to the gas mass above some density threshold fail to match at least some of the data.
20 pages, 4, figures, 4 tables, emulateapj format, accepted to ApJ. This version fixes a minor error in equation 18; no other changes
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- Unveiling the role of galactic rotation on star formation
- APEX-SEPIA660 Early Science: Gas at densities above cm towards OMC-1
- Connecting the Cosmic Star Formation Rate with the Local Star Formation
- Simulated observations of star formation regions: infrared evolution of globally collapsing clouds
- ALMA Observations of HCO+ and HCN Emission in a massive star forming region N55 of the Large Magellanic Cloud
- Origin of the Galaxy Mass-Metallicity-Star-Formation Relation
- The density gradient inside molecular-gas clumps as a booster of their star formation activity
- The Anatomy of a Star-Forming Galaxy II: the role of FUV heating via dust
- Spitzer IRAC identification of Herschel-ATLAS SPIRE sources
- Low star formation efficiency due to turbulent adiabatic compression in the Taffy bridge
- Redshift Evolution of the H2/HI Mass Ratio In Galaxies
- Reconstructing three-dimensional densities from two-dimensional observations of molecular gas
- Investigating the ultraviolet and infrared radiation through the turbulent life of molecular clouds
- The life cycle of starbursting circumnuclear gas discs
- The THESAN-ZOOM project: Star-formation efficiencies in high-redshift galaxies
- Radio halos of star forming galaxies
- When Gas Dynamics Decouples from Galactic Rotation: Characterizing ISM Circulation in Disk Galaxies
- Galaxy And Mass Assembly (GAMA): Gas Fuelling of Spiral Galaxies in the Local Universe II. -- Direct Measurement of the Dependencies on Redshift and Host Halo Mass of Stellar Mass Growth in Central Disk Galaxies
- Probing the link between quenching and morphological evolution
- Cosmological Constraints on the Global Star Formation Law of Galaxies: Insights From Baryon Acoustic Oscillation Intensity Mapping
- Physical Properties and Scaling Relations of Molecular Clouds: the Impact of Star Formation
- Is this an Early Stage Merger? A Case Study on Molecular Gas and Star Formation Properties of Arp 240
- Can the removal of molecular cloud envelopes by external feedback affect the efficiency of star formation?
- The growth of disks and bulges during hierarchical galaxy formation. II: metallicity, stellar populations and dynamical evolution
- Probing the Global Dust Properties and Cluster Formation Potential of the Giant Molecular Cloud G148.24+00.41
- Does the HCN/CO ratio trace the star-forming fraction of gas? I. A comparison with analytical models of star formation
- Modelling H and its effects on star formation using a joint implementation of GADGET-3 and KROME
- A Virgo Environmental Survey Tracing Ionised Gas Emission (VESTIGE) XVII. Statistical properties of individual HII regions in unperturbed systems
- The THESAN-ZOOM project: Star formation efficiency from giant molecular clouds to galactic scale in high-redshift starbursts
- The Environments of CO Cores and Star Formation in the Dwarf Irregular Galaxy WLM
- VALES V: A kinematic analysis of the molecular gas content in -ATLAS galaxies at using ALMA
- On the Functional Form of the Universal Star Formation Law
- Dark-ages reionization and galaxy formation simulation - IX. Economics of reionizing galaxies
- Kinematics of Subclusters in Star Cluster Complexes: Imprint of their Parental Molecular Clouds
- A physical model for the redshift evolution of high-z Lyman-Break Galaxies
- Variations of the ISM Compactness Across the Main Sequence of Star-Forming Galaxies: Observations and Simulations
- The disk averaged star formation relation for Local Volume dwarf galaxies
- The Physical Nature of the Most Metal-Poor Damped Lyman Alpha Systems
- Predicting HCN, HCO + , multi-transition CO, and dust emission of star-forming galaxies: Constraining the properties of resolved gas and dust disks of local spiral galaxies
- Interaction between the Supernova Remnant W44 and the Infrared Dark Cloud G034.77-00.55: shock induced star formation?
- Die Hard: The On-Off-Cycle of Galaxies on the Star Formation Main Sequence
- Gravity or turbulence? VII. The Schmidt-Kennicutt law, the star formation efficiency, and the mass density of clusters from gravitational collapse rather than turbulent support
- Unveiling the gravitationally unstable disc of a massive star-forming galaxy using NOEMA and MUSE
- Exploring extreme conditions for star formation: a deep search for molecular gas in the Leo ring
- A cautionary note about composite Galactic star formation relations
- Gas Accretion and Star-Formation Rates with IFUs and Background Quasars
- An H kinematic survey of the Reference Survey -- I. Fabry-Perot observations with the 1.93m telescope at OHP
- A 260 pc resolution ALMA map of HCN(1-0) in the galaxy NGC 4321
- Molecular clumps disguising their star formation efficiency per freefall time: What we can do not to be fooled
- The Volumetric Extended-Schmidt Law: A Unity Slope
- Forming Stars in a Dual AGN Host: Molecular and Ionized Gas in the Nearby, Luminous Infrared Merger, Mrk 266
- Predicting HCN, HCO, multi-transition CO, and dust emission of star-forming galaxies -- Extension to luminous infrared galaxies and the role of cosmic ray ionization
- The Volumetric Star Formation Law in the Almost Edge-on Galaxy NGC 4302 Revealed by ALMA
- CHOH as a User-Friendly Density Probe: Calibration and Beyond
- The Hierarchical Dynamical State of Molecular Gas from 3 to 300 pc in NGC 253
- A path towards constraining the evolution of the interstellar medium and outflows in the Milky Way using APOGEE
- The role of environment on the evolution of disc galaxies density profiles New insights from simulations and comparison to Euclid data
- Wind of Change: Faraday Rotation in a Simulated Large Magellanic Cloud
- The Relative Importance of Thermal Gas, Radiation, and Magnetic Pressures Around Star-Forming Regions in Normal Galaxies and Dusty Starbursts
- Feedback Regulated Turbulence, Magnetic Fields, and Star Formation Rates in Galactic Disks
- The universality of the relation between magnetic fields and star formation in galaxies
- Discovery of new N-emitters over a wide redshift range
- The Star Formation Factory revisited I. The impact of metallicity on collapsing star-forming clouds
- Fire from Ice - Massive Star Birth from Infrared Dark Clouds
- Galaxy Properties at the Faint End of the HI Mass Function
- Molecular line ratio diagnostics and gas kinematics in the AGN host Seyfert galaxy NGC 5033
- Investigating the role of turbulence in the interstellar medium in dusty star-forming galaxies using kpc-resolution ALMA dust and gas maps
- Formation of stars and clusters over cosmological time
- Atmospheric pressure and molecular cloud formation in early-type galaxies
- Modes of star formation from Herschel
- Numerical Modeling of Multiphase, Turbulent Galactic Disks with Star Formation Feedback
- The Dense Gas Mass Fraction and the Relationship to Star Formation in M51
- Photoevaporation of protoplanetary disks by Far-UV photons arising from neighbouring massive stars: observation of proplyds and modelling
- EMBERS I: Low redshift post-starburst galaxies are frequently depleted in molecular gas relative to star forming progenitors
- The Interstellar Medium and Star Formation in Dwarf Galaxies
- The importance of the way in which supernova energy is distributed around young stellar populations in simulations of galaxies
- Theoretical considerations for star formation at low and high redshift
- Star-formation laws in extreme starbursts