Turbulent Gas in Lensed Planck-selected Starbursts at redshifts 1-3.5
arXiv:2010.16231 · doi:10.3847/1538-4357/abcc01
Abstract
Dusty star-forming galaxies at high redshift (1 < z < 3) represent the most intense star-forming regions in the Universe. Key aspects to these processes are the gas heating and cooling mechanisms. Although it is well known that these galaxies are gas-rich, little is known about the gas excitation conditions. Here we examine these processes in a sample of 24 strongly lensed star-forming galaxies identified by the \textit{Planck} satellite (LPs) at z ~ 1.1 - 3.5. We analyze 162 CO rotational transitions (ranging from Jupper = 1 - 12) and 37 atomic carbon fine-structure lines ([CI]) in order to characterize the physical conditions of the gas in sample of LPs. We simultaneously fit the CO and [CI] lines, and the dust continuum emission, using two different non-LTE, radiative transfer models. The first model represents a two component gas density, while the second assumes a turbulence driven log-normal gas density distribution. These LPs are among the most gas-rich, infrared (IR) luminous galaxies ever observed (L\Lsun; M \Msun, with the average lens magnification factor). Our results suggest that the turbulent ISM present in the LPs can be well-characterized by a high turbulent velocity dispersion ( \kms) and gas kinetic temperature to dust temperature ratios /, sustained on scales larger than a few kpc. We speculate that the average surface density of the molecular gas mass and IR luminosity \Msun pc and \Lsun kpc, arise from both stellar mechanical feedback and a steady momentum injection from the accretion of intergalactic gas.
arXiv comment54 pages, 18 figures. Accepted for publication in The Astrophysical Journal (as of Oct. 30, 2020). Please feel free to view the supplementary figures here (which can later be found online in the ApJ after the full publication procedure): https://drive.google.com/drive/folders/1CN3rqlUDcNi5JSDH2GhFk_SLSlo10han?usp=sharing
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- PRUSSIC I - a JVLA survey of HCN/HCO+/HNC (1-0) emission in z3 dusty galaxies: Low dense-gas fractions in high-redshift star-forming galaxies
- PASSAGES: The Large Millimeter Telescope and ALMA Observations of Extremely Luminous High Redshift Galaxies Identified by the Planck
- Observations of neutral carbon in 29 high-z lensed dusty star forming galaxies and the comparison of gas mass tracers
- The effect of active galactic nuclei on the cold interstellar medium in distant star-forming galaxies
- z-GAL -- A NOEMA spectroscopic redshift survey of bright Herschel galaxies: [III] Physical properties
- Molecular gas and star formation in nearby starburst galaxy mergers
- High resolution spectral imaging of CO(7-6), [CI](2-1) and continuum of three high-z lensed dusty star-forming galaxies using ALMA
- Resolved CO(1-0) emission and gas properties in luminous dusty star forming galaxies at z=2-4
- The cold interstellar medium of a normal sub- galaxy at the end of reionization
- Modelling high-resolution ALMA observations of strongly lensed dustystar forming galaxies detected by Herschel
- Unveiling the warm dense ISM in quasar host galaxies via water vapor emission
- The cold molecular gas in z6 quasar host galaxies
- APEX at the QSO MUSEUM: molecular gas reservoirs associated with 3 quasars and their link to the extended Ly emission
- Molecular gas properties of Q1700-MD94: a massive, main-sequence galaxy at
- A search for candidate strongly-lensed dusty galaxies in the Planck satellite catalogues
- High-z Sudoku: A diagnostic tool for identifying robust (sub)mm redshifts
- CI and CO in Nearby Spiral Galaxies -- I. Line Ratio and Abundance Variations at ~ 200 pc Scales
- Metallicity dependence of the CO-to-H and the [CI]-to-H conversion factors in galaxies
- CO Excitation and Line Energy Distributions in Gas-selected Galaxies
- HYACINTH: HYdrogen And Carbon chemistry in the INTerstellar medium in Hydro simulations
- Ionized Carbon in Galaxies: The [C II] 158 m Line as a Total Molecular Gas Mass Tracer Revisited
- Revealing the hidden cosmic feast: A z=4.3 galaxy group hosting two optically dark, efficiently star-forming galaxies
- PRUSSIC II -- ALMA imaging of dense-gas tracers in SDP.81: Evidence for low mechanical heating and a sub-solar metallicity in a z=3.04 dusty galaxy
- CO Excitation in High-z Main Sequence Analogues: Resolved CO(4-3)/CO(3-2) Line Ratios in DYNAMO Galaxies
- Massive molecular gas reservoir in a luminous sub-millimeter galaxy during cosmic noon
- CO(1--0) imaging reveals 10-kiloparsec molecular gas reservoirs around star-forming galaxies at high redshift
- Milky Way-Like Gas Excitation in an Ultrabright Submillimeter Galaxy at
- DESHIMA 2.0: Rapid redshift surveys and multi-line spectroscopy of dusty galaxies
- PRUSSIC III -- ALMA and NOEMA survey of dense gas in high-redshift star-forming galaxies
- The Einstein ring GAL-CLUS-022058s: a Lensed Ultrabright Submillimeter Galaxy at z=1.4796
- "Dust Giant": Extended and Clumpy Star-Formation in a Massive Dusty Galaxy at
- A possible relation between global CO excitation and massive molecular outflows in local ULIRGs
- Formation of Substructure in Luminous Submillimeter Galaxies (FOSSILS): Evidence of Multiple Pathways to Trigger Starbursts in Luminous Submillimeter Galaxies
- Vz-GAL: Probing Cold Molecular Gas in Dusty Star-forming Galaxies at z=1-6
- Hot Diggity Dog: Simultaneous CO and Dust Modeling of the Most Luminous WISE Hot Dust-Obscured Galaxy Unveils Extreme Molecular Gas Excitation
- PASSAGES: The Discovery of a Strongly Lensed Protocluster Core Candidate at Cosmic Noon
- Molecular gas content and high excitation of a massive main-sequence galaxy at z = 3
- Tight correlation of star formation with [Ci] and CO lines across cosmic time
- Direct detection of cool molecular gas in a star-forming galaxy at
- Measuring the HI content of individual galaxies out to the epoch of reionization with [CII]
- GRB host galaxies with strong H absorption: CO-dark molecular gas at the peak of cosmic star formation
- Predicting the resolved CO emission of star-forming galaxies
- Hiding behind a curtain of dust: Gas and dust properties of an ultra-luminous strongly-lensed z = 3.75 galaxy behind the Milky Way disk
- Possible Ongoing Merger Discovered by Photometry and Spectroscopy in the Field of the Galaxy Cluster PLCK G165.7+67.0
- The LMT 2 Millimeter Receiver System (B4R). I. Overview and Results of Science Demonstration
- Kiloparsec-scale imaging of the CO(1-0)-traced cold molecular gas reservoir in a z~3.4 submillimeter galaxy