ALMA view of RX J1131-1231: Sub-kpc CO (2-1) mapping of a molecular disk in a lensed star-forming quasar host galaxy
arXiv:1705.09931 · doi:10.1051/0004-6361/201731250
Abstract
We present ALMA 2-mm continuum and CO (2-1) spectral line imaging of the gravitationally lensed z=0.654 star-forming/quasar composite RX J1131-1231 at 240-400 mas angular resolution. The continuum emission is found to be compact and coincident with the optical emission, whereas the molecular gas forms a complete Einstein ring, which shows strong differential magnification. The de-lensed source structure is determined on 400-pc resolution using a visibility-fitting lens modelling technique. The reconstructed molecular gas velocity-field is consistent with a rotating disk with a maximum rotational velocity of 280 km/s. From dynamical model fitting we find an enclosed mass M(r<5 kpc)=(1.46+/-0.31)*10^11 M_sol. The molecular gas distribution is highly structured, with clumps that are co-incident with higher gas velocity dispersion regions 40-50 km/s and with the intensity peaks in the optical emission, which are associated with sites of on-going turbulent star-formation. The peak in the CO (2-1) distribution is not co-incident with the AGN, where there is a paucity of molecular gas emission, possibly due to radiative feedback from the central engine. The intrinsic molecular gas luminosity is L'_CO=(1.2+/-0.3)*10^10 K km/s pc^2 and the inferred gas mass is M(H2)=(8.3+/-3.0)*10^10 M_sol, which given its dynamical mass is consistent with a CO-H2 conversion factor of alpha = 5.5+/-2.0 M_solar(K km/s pc^2)^-1. This suggests that the star-formation efficiency is dependent on the host galaxy morphology as opposed to the nature of the AGN. The far-infrared continuum spectral energy distribution shows evidence for heated dust, equivalent to an obscured star-formation rate of SFR=69^(+41)_(-25)*(7.3/u_IR)M_sol/yr, which demonstrates the composite star-forming/AGN nature of this system. RX J1131-1231
arXiv comment12 pages, 8 figures, accepted by A&A
References in corpus (37)
- Planck 2015 results. XIII. Cosmological parameters
- The Star Formation Efficiency in Nearby Galaxies: Measuring Where Gas Forms Stars Effectively
- The Molecular Interstellar Medium in Ultraluminous Infrared Galaxies
- Very High Gas Fractions and Extended Gas Reservoirs in z=1.5 Disk Galaxies
- Molecular Gas at High Redshift
- Submillimeter Galaxies at z~2: Evidence for Major Mergers & Constraints on Lifetimes, IMF and CO-H2 Conversion Factor
- An interferometric CO survey of luminous submm galaxies
- H0LiCOW V. New COSMOGRAIL time delays of HE0435-1223: to 3.8% precision from strong lensing in a flat CDM model
- Two accurate time-delay distances from strong lensing: Implications for cosmology
- H0LiCOW I. Lenses in COSMOGRAIL's Wellspring: Program Overview
- Bayesian Strong Gravitational-Lens Modeling on Adaptive Grids: Objective Detection of Mass Substructure in Galaxies
- Cosmology from gravitational lens time delays and Planck data
- The Sizes of the X-ray and Optical Emission Regions of RXJ1131-1231
- Highly-excited CO emission in APM08279+5255 at z=3.9
- CO(1-0) in z>2 Quasar Host Galaxies: No Evidence for Extended Molecular Gas Reservoirs
- CO(1-0) in z >/~ 4 Quasar Host Galaxies: No Evidence for Extended Molecular Gas Reservoirs
- ALMA reveals the feeding of the Seyfert 1 nucleus in NGC 1566
- COSMOGRAIL: the COSmological MOnitoring of GRAvItational Lenses XIII: Time delays and 9-yr optical monitoring of the lensed quasar RX J1131-1231
- A CO emission line from the optical and near-IR undetected submillimeter galaxy GN10
- A quadruply imaged quasar with an optical Einstein ring candidate: 1RXS J113155.4-123155
- ALMA Long Baseline Observations of the Strongly Lensed Submillimeter Galaxy HATLAS J090311.6+003906 at z=3.042
- The mass-sheet degeneracy and time-delay cosmography: Analysis of the strong lens RXJ1131-1231
- The JCMT Nearby Galaxies Legacy Survey I. Star Forming Molecular Gas in Virgo Cluster Spiral Galaxies
- Multi-wavelength study of the gravitational lens system RXS J1131-1231: III. Long slit spectroscopy: micro-lensing probes the QSO structure
- A Total Molecular Gas Mass Census in z~2-3 Star-forming Galaxies: Low-J CO Excitation Probes of Galaxies' Evolutionary States
- A Molecular Einstein Ring at z=4.12: Imaging the Dynamics of a Quasar Host Galaxy Through a Cosmic Lens
- Revealing the Structure of an Accretion Disk Through Energy Dependent X-ray Microlensing
- SHARP - III: First Use Of Adaptive Optics Imaging To Constrain Cosmology With Gravitational Lens Time Delays
- Herschel-SPIRE, Far-Infrared Properties of Millimetre-Bright and -Faint Radio Galaxies
- ALMA imaging of SDP.81 - II. A pixelated reconstruction of the CO emission lines
- Multi wavelength study of the gravitational lens system RXS J1131-1231: II Lens model and source reconstruction
- Gravitational lensing reveals extreme dust-obscured star formation in quasar host galaxies
- Reflection From the Strong Gravity Regime in a z=0.658 Gravitationally Lensed-Quasar
- Molecular Gas in the z=1.2 Ultraluminous Merger GOODS J123634.53+621241.3
- Integral Field Spectroscopy of the Quadruply Lensed Quasar 1RXS J1131-1231: New Light on Lens Substructures
- Multi-wavelength study of the gravitational lens system RXS J113155.4-123155: I. Multi-epoch optical and near infrared imaging
- Molecular Gas Kinematics and Star Formation Properties of the Strongly-Lensed Quasar Host Galaxy RXS J1131-1231
Cited by in corpus (18)
- SUPER IV. CO(J=3-2) properties of active galactic nucleus hosts at cosmic noon revealed by ALMA
- Strong lensing in UNIONS: Toward a pipeline from discovery to modeling
- SHARP -- VI. Evidence for CO (1-0) molecular gas extended on kpc-scales in AGN star forming galaxies at high redshift
- A Survey for High-redshift Gravitationally Lensed Quasars and Close Quasars Pairs. I. the Discoveries of an Intermediately-lensed Quasar and a Kpc-scale Quasar Pair at
- A Mock Catalog of Gravitationally Lensed Quasars for the LSST Survey
- A flux-ratio anomaly in the CO spectral line emission from gravitationally-lensed quasar MG J0414+0534
- Euclid: The Early Release Observations Lens Search Experiment
- VLA and ALMA observations of the lensed radio-quiet quasar SDSS J0924+0219: a molecular structure in a 3 microJy radio source
- J17218842: a gravitationally lensed binary quasar with a proximate damped Lyman- absorber
- Duality in spatially resolved star-formation relations in local LIRGs
- Linking the small scale relativistic winds and the large scale molecular outflows in the z = 1.51 lensed quasar HS 0810+2554
- High resolution spectral imaging of CO(7-6), [CI](2-1) and continuum of three high-z lensed dusty star-forming galaxies using ALMA
- Gravitational lensing in LoTSS DR2 -- Extremely faint 144-MHz radio emission from two highly magnified quasars
- Resolving Complex Inner X-ray Structure of the Gravitationaly Lensed AGN MGB2016+112
- Detection of millimeter-wave coronal emission in a quasar at cosmological distance using microlensing
- Multi-scale VLBI observations of the candidate host galaxy of GRB 200716C
- Molecular gas content of gravitational-lensed quasars at cosmic noon
- Using strong lensing to understand the microJy radio emission in two radio quiet quasars at redshift 1.7