Evidence for a non-universal Kennicutt-Schmidt relationship using hierarchical Bayesian linear regression
arXiv:1210.1218 · doi:10.1093/mnras/sts617
Abstract
For investigating the relationship between the star formation rate and gas surface density, we develop a Bayesian linear regression method that rigorously treats measurement uncertainties and accounts for hierarchical data structure. The hierarchical method simultaneously estimates the intercept, slope, and scatter about the regression line of each individual subject and the population. Using synthetic datasets, we demonstrate that the method recovers the underlying parameters of both the individuals and the population, especially when compared to commonly employed ordinary least squares techniques, such as the bisector fit. We apply the hierarchical method to estimate the Kennicutt-Schmidt (KS) parameters of a sample of spiral galaxies compiled by Bigiel et al. (2008). We find significant variation in the KS parameters, indicating that no single relationship holds for all galaxies. This suggests that the relationship between molecular gas and star formation differs between galaxies, possibly due to the influence of other properties within a given galaxy, such as metallicity, molecular gas fraction, or stellar mass. In four galaxies the slope estimates are sub-linear (at the 95% level). We estimate the mean index of the KS relationship for the population to be 0.84, with 95% range [0.63, 1.0]. For the galaxies with sub-linear KS relationships, a possible interpretation is that CO emission is tracing some molecular gas that is not directly associated with star formation. Equivalently, a sub-linear KS relationship may be indicative of an increasing gas depletion time at higher surface densities, as traced by CO emission. The Bayesian method can account for all sources of uncertainties, including variations in the conversion of observed intensities to star formation rates and gas surface densities, and is therefore well suited for a thorough statistical analysis of the KS law.
17 pages, 3 figures, 8 tables, Accepted to MNRAS - updated to match accepted version. (Abstract abridged)
References in corpus (17)
- Theory of Star Formation
- Some Aspects of Measurement Error in Linear Regression of Astronomical Data
- The GALEX Ultraviolet Atlas of Nearby Galaxies
- The Star Formation Rate of Turbulent Magnetized Clouds: Comparing Theory, Simulations, and Observations
- Star Formation and Feedback in Smoothed Particle Hydrodynamic Simulations--I. Isolated Galaxies
- COLD GASS, an IRAM Legacy Survey of Molecular Gas in Massive Galaxies: II. The non-universality of the Molecular Gas Depletion Timescale
- Simulating the formation of molecular clouds. I. Slow formation by gravitational collapse from static initial conditions
- Simulating the formation of molecular clouds. II. Rapid formation from turbulent initial conditions
- Inferring the eccentricity distribution
- The linewidth-size relationship in the dense ISM of the Central Molecular Zone
- How long does it take to form a molecular cloud?
- A Survey of Galaxy Kinematics to z ~ 1 in the TKRS/GOODS-N Field. II. Evolution in the Tully-Fisher Relation
- Maximally Star-Forming Galactic Disks II. Vertically-Resolved Hydrodynamic Simulations of Starburst Regulation
- Cloud and Star Formation in Disk Galaxy Models with Feedback
- Star Formation Laws: the Effects of Gas Cloud Sampling
- How Universal is the SFR - H2 Relation?
- Evidence for Grain Growth in Molecular Clouds: A Bayesian Examination of the Extinction Law in Perseus
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- The SILCC (SImulating the LifeCycle of molecular Clouds) project: I. Chemical evolution of the supernova-driven ISM
- The Big Problems in Star Formation: the Star Formation Rate, Stellar Clustering, and the Initial Mass Function
- The SILCC (SImulating the LifeCycle of molecular Clouds) project - II. Dynamical evolution of the supernova-driven ISM and the launching of outflows
- On the [CII]-SFR relation in high redshift galaxies
- Cloud Scale ISM Structure and Star Formation in M51
- Deriving a multivariate CO-to-H conversion function using the [CII]/CO(1-0) ratio and its application to molecular gas scaling relations
- Variations of the stellar initial mass function in the progenitors of massive early-type galaxies and in extreme starburst environments
- What FIREs Up Star Formation: the Emergence of the Kennicutt-Schmidt Law from Feedback
- The ATLAS3D project - XXII. Low-efficiency star formation in early-type galaxies: hydrodynamic models and observations
- Black Hole Mass Scaling Relations for Spiral Galaxies. I. -
- Distribution and mass of diffuse and dense CO gas in the Milky Way
- The Dense Gas Mass Fraction of Molecular Clouds in the Milky Way
- The origin of physical variations in the star formation law
- The ALMaQUEST Survey: V. The non-universality of kpc-scale star formation relations and the factors that drive them
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- Re-visiting the extended Schmidt law: the important role of existing stars in regulating star formation
- A physical model for the [CII]-FIR deficit in luminous galaxies
- Radial gas motions in The HI Nearby Galaxy Survey (THINGS)
- On column density thresholds and the star formation rate
- Sub-kiloparsec Imaging of Cool Molecular Gas in Two Strongly Lensed Dusty, Star-Forming Galaxies
- Star Formation On Sub-kpc Scale Triggered By Non-linear Processes In Nearby Spiral Galaxies
- The resolved star-formation relation in nearby active galactic nuclei
- A panchromatic spatially resolved analysis of nearby galaxies -- II. The main sequence - gas relation at sub-kpc scale in grand-design spirals
- Star formation laws in the Andromeda galaxy: gas, stars, metals and the surface density of star formation
- Collapse in Self-gravitating Turbulent Fluids
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- Spatially-Resolved Dense Molecular Gas and Star Formation Rate in M51
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- Type Ia Supernova Colors and Ejecta Velocities: Hierarchical Bayesian Regression with Non-Gaussian Distributions
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- Molecular Cloud-scale Star Formation in NGC 300
- Lessons from cosmic history: The case for a linear star formation -- H2 relation
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- The role of turbulence in star formation laws and thresholds
- The variation in molecular gas depletion time among nearby galaxies: II the impact of galaxy internal structures
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- Damped Lyα Absorption Systems in Semi-Analytic Models with Multiphase Gas
- Star formation efficiencies of molecular clouds in a galactic center environment
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- The Dense Gas Mass Fraction and the Relationship to Star Formation in M51
- The link between star formation and gas in nearby galaxies