Molecular Gas, Dust and Star Formation in Galaxies: II. Dust properties and scalings in \sim\ 1600 nearby galaxies
arXiv:1703.09829 · doi:10.1051/0004-6361/201629009
Abstract
We aim to characterize the relationship between dust properties. We also aim to provide equations to estimate accurate dust properties from limited observational datasets. We assemble a sample of 1,630 nearby (z<0.1) galaxies-over a large range of Mstar, SFR - with multi-wavelength observations available from wise, iras, planck and/or SCUBA. The characterization of dust emission comes from SED fitting using Draine & Li dust models, which we parametrize using two components (warm and cold ). The subsample of these galaxies with global measurements of CO and/or HI are used to explore the molecular and/or atomic gas content of the galaxies. The total Lir, Mdust and dust temperature of the cold component (Tc) form a plane that we refer to as the dust plane. A galaxy's sSFR drives its position on the dust plane: starburst galaxies show higher Lir, Mdust and Tc compared to Main Sequence and passive galaxies. Starburst galaxies also show higher specific Mdust (Mdust/Mstar) and specific Mgas (Mgas/Mstar). The Mdust is more closely correlated with the total Mgas (atomic plus molecular) than with the individual components. Our multi wavelength data allows us to define several equations to estimate Lir, Mdust and Tc from one or two monochromatic luminosities in the infrared and/or sub-millimeter. We estimate the dust mass and infrared luminosity from a single monochromatic luminosity within the R-J tail of the dust emission, with errors of 0.12 and 0.20dex, respectively. These errors are reduced to 0.05 and 0.10 dex, respectively, if the Tc is used. The Mdust is correlated with the total Mism (Mism \propto Mdust^0.7). For galaxies with Mstar 8.5<log(Mstar/Msun) < 11.9, the conversion factor α_850mum shows a large scatter (rms=0.29dex). The SF mode of a galaxy shows a correlation with both the Mgass and Mdust: high Mdust/Mstar galaxies are gas-rich and show the highest SFRs.
arXiv comment24 pages, 28 figures, 6 tables, Accepted for publication in A&A
References in corpus (88)
- Star Formation in Galaxies Along the Hubble Sequence
- The Origin of the Mass--Metallicity Relation: Insights from 53,000 Star-Forming Galaxies in the SDSS
- Star Formation in the Milky Way and Nearby Galaxies
- Stellar Masses and Star Formation Histories for 10^5 Galaxies from the Sloan Digital Sky Survey
- Interstellar Dust Grains
- The Optical and Near-Infrared Properties of Galaxies: I. Luminosity and Stellar Mass Functions
- The CO-to-H2 Conversion Factor
- Infrared Emission from Interstellar Dust. IV. The Silicate-Graphite-PAH Model in the Post-Spitzer Era
- Star Formation in AEGIS Field Galaxies since z=1.1 : The Dominance of Gradually Declining Star Formation, and the Main Sequence of Star-Forming Galaxies
- The reversal of the star formation-density relation in the distant universe
- Rotating Nuclear Rings and Extreme Starbursts in Ultraluminous Galaxies
- SINGS: The SIRTF Nearby Galaxies Survey
- A simple model to interpret the ultraviolet, optical and infrared emission from galaxies
- The Atlas3D project -- I. A volume-limited sample of 260 nearby early-type galaxies: science goals and selection criteria
- GOODS-Herschel: an infrared main sequence for star-forming galaxies
- Cool Gas in High Redshift Galaxies
- Dust Masses, PAH Abundances, and Starlight Intensities in the SINGS Galaxy Sample
- The Molecular Interstellar Medium in Ultraluminous Infrared Galaxies
- Spectral Energy Distributions of Hard X-ray selected AGNs in the XMDS Survey
- Molecular Gas at High Redshift
- The lesser role of starbursts for star formation at z=2
- Calibrating Extinction-Free Star Formation Rate Diagnostics with 33GHz Free-Free Emission in NGC6946
- The Herschel view of the dominant mode of galaxy growth from z=4 to the present day
- SCUBA: A common-user submillimetre camera operating on the James Clerk Maxwell Telescope
- The 2MASS Redshift Survey - Description and Data Release
- The Arecibo Legacy Fast ALFA Survey: The alpha.40 HI Source Catalog, its Characteristics and their Impact on the Derivation of the HI Mass Function
- Combined CO & Dust Scaling Relations of Depletion Time and Molecular Gas Fractions with Cosmic Time, Specific Star Formation Rate and Stellar Mass
- The HIPASS Catalogue - I. Data Presentation
- Determining Star Formation Rates for Infrared Galaxies
- The CO-to-H2 Conversion Factor and Dust-to-Gas Ratio on Kiloparsec Scales in Nearby Galaxies
- The Herschel ATLAS
- The CO-to-H2 Conversion Factor From Infrared Dust Emission Across the Local Group
- Improved background subtraction for the Sloan Digital Sky Survey images
- Optical Spectroscopy and Nebular Oxygen Abundances of the Spitzer/SINGS Galaxies
- The SCUBA Local Universe Galaxy Survey I: First Measurements of the Submillimetre Luminosity and Dust Mass Functions
- The Las Campanas Redshift Survey
- The 1000 Brightest HIPASS Galaxies: HI Properties
- ISM masses and the star formation law at Z = 1 to 6 // ALMA observations of dust continuum in 145 galaxies in the COSMOS survey field
- A Digital Archive of HI 21 cm Line Spectra of Optically-targeted Galaxies
- The Atlas3D project -- IV: the molecular gas content of early-type galaxies
- The SCUBA Local Universe Galaxy Survey II. 450 micron data - evidence for cold dust in bright IRAS Galaxies
- Extending the Nearby Galaxy Heritage with WISE: First Results from the WISE Enhanced Resolution Galaxy Atlas
- The evolution of the dust and gas content in galaxies
- The Evolution of ISM Mass Probed by Dust Emission -- ALMA Observations at z = 0.3 to 2
- Predicting dust extinction from the stellar mass of a galaxy
- Herschel Far-Infrared and Sub-millimeter Photometry for the KINGFISH Sample of Nearby Galaxies
- Stellar Masses and SFRs for 1M Galaxies from SDSS and WISE
- Infrared Spectral Energy Distributions of Nearby Galaxies
- Herschel-ATLAS: Rapid evolution of dust in galaxies in the last 5 billion years
- Galaxy And Mass Assembly (GAMA): Mid-Infrared Properties and Empirical Relations from
- Global Star Formation Rates in Disk Galaxies and Circumnuclear Starbursts from Cloud Collisions
- The molecular gas in Luminous Infrared Galaxies I: CO lines, extreme physical conditions, and their drivers
- The dust scaling relations of the Herschel Reference Survey
- The HIPASS Catalogue: III - Optical Counterparts & Isolated Dark Galaxies
- GOODS-HERSCHEL: star formation, dust attenuation and the FIR-radio correlation on the Main Sequence of star-forming galaxies up to z~4
- Herschel unveils a puzzling uniformity of distant dusty galaxies
- Star formation laws in Luminous Infrared Galaxies. New observational constraints on models
- Dust Spectral Energy Distributions of Nearby Galaxies: an Insight from the Herschel Reference Survey
- The Northern HIPASS catalogue - Data presentation, completeness and reliability measures
- New insight into the relation between star formation activity and dust content in galaxies
- Evidence of enhanced star formation efficiency in luminous and ultraluminous infrared galaxies
- Evolution of Dust Temperature of Galaxies through Cosmic Time as seen by Herschel
- Herschel-ATLAS: Multi-wavelength SEDs and physical properties of 250 micron-selected galaxies at z < 0.5
- The Arecibo Legacy Fast ALFA Survey: IV. Strategies for Signal Identification and Survey Catalog Reliability
- Modeling Dust and Starlight in Galaxies Observed by Spitzer and Herschel: NGC 628 and NGC 6946
- Cold Molecular Gas in Merger Remnants: I. Formation of Molecular Gas Disks
- Dust and star-formation properties of a complete sample of local galaxies drawn from the Planck Early Release Compact Source Catalogue
- The Submillimetre Properties of Ultraluminous Infrared Galaxies
- Dust and gas in luminous proto-cluster galaxies at z=4.05: the case for different cosmic dust evolution in normal and starburst galaxies
- The Herschel Virgo Cluster Survey: X.The relationship between cold dust and molecular gas content in Virgo spirals
- Far-infrared surveys of galaxy evolution
- The Arecibo Legacy Fast ALFA Survey: II. Results of Precursor Observations
- The JCMT Nearby Galaxies Legacy Survey VIII. CO data and the L(CO3-2)-L(FIR) correlation in the SINGS sample
- An Extragalactic 12CO J=3-2 survey with the Heinrich-Hertz-Telescope
- FIR colours and SEDs of nearby galaxies observed with Herschel
- First Results from the HI Jodrell All Sky Survey: Inclination-Dependent Selection Effects in a 21-cm Blind Survey
- Far-infrared properties of submillimeter and optically faint radio galaxies
- A Multi-wavelength View of the Star Formation Activity at z~3
- The Arecibo Legacy Fast ALFA Survey: VI. Second HI Source Catalog of the Virgo Cluster Region
- Herschel-ATLAS: The Surprising Diversity of Dust-Selected Galaxies in the Local Submillimetre Universe
- A new infrared color criterion for the selection of 0<z<7 AGN: application to deep fields and implications for JWST surveys
- Isothermal dust models of Herschel-ATLAS galaxies
- The local luminosity function of star-forming galaxies derived from the Planck Early Release Compact Source Catalogue
- The infrared compactness-temperature relation for quiescent and starburst galaxies
- The Arecibo Legacy Fast ALFA Survey: V. HI Source Catalog of the Anti-Virgo Region at dec=27 degrees
- 12co(J=1-0) on-the-Fly Mapping Survey of the Virgo Cluster Spirals. I. Data and Atlas
- The Arecibo Legacy Fast ALFA Survey: VIII. HI Source Catalog of the Anti-Virgo Region at dec = +25 deg
- The Herschel Virgo Cluster Survey. XIX. Physical properties of low luminosity FIR sources at 0.5
Cited by in corpus (34)
- Comprehensive comparison of models for spectral energy distributions from 0.1 micron to 1 mm of nearby star-forming galaxies
- Dust, CO and [CI]: Cross-calibration of molecular gas mass tracers in metal-rich galaxies across cosmic time
- The ISM scaling relations in DustPedia late-type galaxies: A benchmark study for the Local Universe
- A panchromatic spatially resolved analysis of nearby galaxies -- II. The main sequence - gas relation at sub-kpc scale in grand-design spirals
- The ALPINE-ALMA [CII] survey: Dust mass budget in the early Universe
- The hidden side of cosmic star formation at z > 3: Bridging optically-dark and Lyman break galaxies with GOODS-ALMA
- Dust continuum, CO, and [C I] 1-0 lines: self-consistent H2 mass estimates and the possibility of globally CO-dark galaxies at
- An evolving and mass dependent - relation for galaxies
- Spectro-photometric decomposition of galaxy structural components
- Spatially resolved dust properties and quasar-galaxy decomposition of a HyLIRG at z = 4.4
- The resolved scaling relations in DustPedia: Zooming in on the local Universe
- The molecular gas properties in local Seyfert 2 galaxies
- The post-Herschel view of intrinsic AGN emission: constructing templates for galaxy and AGN emission at IR wavelengths
- Dissecting Nearby Galaxies with piXedfit: II. Spatially Resolved Scaling Relations Among Stars, Dust, and Gas
- Using Host Galaxy Spectroscopy to Explore Systematics in the Standardisation of Type Ia Supernovae
- Dust Attenuation Curves at z 0.8 from LEGA-C: Precise Constraints on the Slope and 2175 Bump Strength
- Quantifying the cool ISM in radio AGNs: evidence for late-time re-triggering by galaxy mergers and interactions
- Modelling the evolution and influence of dust in cosmological simulations that include the cold phase of the interstellar medium
- Cold gas and dust: Hunting spiral-like structures in early-type galaxies
- Variation of optical and infrared properties of galaxies with their surface brightness
- Probing star formation and ISM properties using galaxy disk inclination III: Evolution in dust opacity and clumpiness between redshift 0.0 < z < 0.7 constrained from UV to NIR
- The local Universe in the era of large surveys -- II. Multi-wavelength characterisation of activity in nearby S0 galaxies
- The Evolution of Brightest Cluster Galaxies in the Nearby Universe II: The star-formation activity and the Stellar Mass from Spectral Energy Distribution
- The ISM scaling relations using inner HI and an application of estimating dust mass
- Cosmic evolution of molecular gas mass density from an empirical relation between and
- Hubble Space Telescope Captures UGC~12591: Bulge/Disc Properties, Star Formation and `Missing Baryons' Census in a Very Massive and Fast Spinning Hybrid Galaxy
- Narrow absorption lines from intervening material in supernovae. II. Galaxy properties
- Relating spatially resolved optical attenuation, dust and gas in nearby galaxies
- Interpreting Millimeter Emission from IMEGIN galaxies NGC 2146 and NGC 2976
- ALMA Lensing Cluster Survey: Dust mass measurements as a function of redshift, stellar-mass and star formation rate, from z=1 to z=5
- Galaxy And Mass Assembly: A new approach to quantifying dust in galaxies
- ALMA Lensing Cluster Survey: average dust, gas, and star formation properties of cluster and field galaxies from stacking analysis
- The role of young and evolved stars in the heating of dust in local galaxies
- The properties of the obscuring material of an AGNs sample from mid-IR and X-ray simultaneous fitting