The depletion of water during dispersal of planet-forming disk regions
arXiv:1611.06230 · doi:10.3847/1538-4357/834/2/152
Abstract
We present a new velocity-resolved survey of 2.9 m spectra of hot HO and OH gas emission from protoplanetary disks, obtained with CRIRES at the VLT ( 3 km s). With the addition of archival Spitzer-IRS spectra, this is the most comprehensive spectral dataset of water vapor emission from disks ever assembled. We provide line fluxes at 2.9-33 m that probe from disk radii of au out to the region across the water snow line. With a combined dataset for 55 disks, we find a new correlation between HO line fluxes and the radius of CO gas emission as measured in velocity-resolved 4.7 m spectra (R), which probes molecular gaps in inner disks. We find that HO emission disappears from 2.9 m (hotter water) to 33 m (colder water) as R increases and expands out to the snow line radius. These results suggest that the infrared water spectrum is a tracer of inside-out water depletion within the snow line. It also helps clarifying an unsolved discrepancy between water observations and models, by finding that disks around stars of M M generally have inner gaps with depleted molecular gas content. We measure radial trends in HO, OH, and CO line fluxes that can be used as benchmarks for models to study the chemical composition and evolution of planet-forming disk regions at 0.05-20 au. We propose that JWST spectroscopy of molecular gas may be used as a probe of inner disk gas depletion, complementary to the larger gaps and holes detected by direct imaging and by ALMA.
arXiv commentAccepted for publication on ApJ
References in corpus (88)
- The Wide-field Infrared Survey Explorer (WISE): Mission Description and Initial On-orbit Performance
- The Spitzer Space Telescope Mission
- Disk Frequencies and Lifetimes in Young Clusters
- The Infrared Spectrograph on the Spitzer Space Telescope
- Some Aspects of Measurement Error in Linear Regression of Astronomical Data
- Planet-disk interaction and orbital evolution
- Resolved Images of Large Cavities in Protoplanetary Transition Disks
- Contributions to the Nearby Stars (NStars) Project: Spectroscopy of Stars Earlier than M0 within 40 parsecs: The Southern Sample
- Observational Constraints on the Formation and Evolution of Binary Stars
- Planet formation around stars of various masses: The snow line and the frequency of giant planets
- Towards a deterministic model of planetary formation. III. Mass distribution of short-period planets around stars of various masses
- Building Terrestrial Planets
- Photoevaporation of protoplanetary discs II: evolutionary models and observable properties
- Radiation thermo-chemical models of protoplanetary disks I. Hydrostatic disk structure and inner rim
- Photoevaporation of Circumstellar Disks by FUV, EUV and X-ray Radiation from the Central Star
- Consistent dust and gas models for protoplanetary disks. I. Disk shape, dust settling, opacities, and PAHs
- Radiation-Hydrodynamic Models of X-Ray & EUV Photoevaporating Protoplanetary Discs
- Which jet launching mechanism(s) in TTauri stars?
- Interstellar water chemistry: from laboratory to observations
- Detection of the Water Reservoir in a Forming Planetary System
- Observational Signatures of Planets in Protoplanetary Disks I: Gaps Opened by Single and Multiple Young Planets in Disks
- Protoplanetary disk lifetimes vs stellar mass and possible implications for giant planet populations
- Transitional and Pre-Transitional disks: Gap Opening by Multiple Planets?
- TEXES: A Sensitive High-Resolution Grating Spectrograph for the Mid-Infrared
- Spectro-astrometric imaging of molecular gas within protoplanetary disk gaps
- H2O and OH gas in the terrestrial planet-forming zones of protoplanetary disks
- Accretion Rates for T Tauri Stars Using Nearly Simultaneous Ultraviolet and Optical Spectra
- A Spitzer survey of mid-infrared molecular emission from protoplanetary disks I: Detection rates
- A spectroscopic survey of Herbig Ae/Be stars with X-Shooter I: Stellar parameters and accretion rates
- Resolved gas cavities in transitional disks inferred from CO isotopologues with ALMA
- Survival of molecular gas in cavities of transition disks (I. CO)
- Towards a Global Evolutionary Model of Protoplanetary Disks
- Dust Migration and Morphology in Optically Thin Circumstellar Gas Disks
- A Spitzer Survey of Mid-Infrared Molecular Emission from Protoplanetary Disks II: Correlations and LTE Models
- The molecular composition of the planet-forming regions of protoplanetary disks across the luminosity regime
- The structure and dynamics of molecular gas in planet-forming zones: A CRIRES spectro-astrometric survey
- The thermal structure and the location of the snow line in the protosolar nebula: axisymmetric models with full 3-D radiative transfer
- Small vs large dust grains in transitional disks: do different cavity sizes indicate a planet?
- On the gas content of transitional disks: a VLT/X-Shooter study of accretion and winds
- Investigating planet formation in circumstellar disks: CARMA observations of RY Tau and DG Tau
- The Impact of Dust Evolution and Photoevaporation on Disk Dispersal
- Warm Gas in the Inner Disks around Young Intermediate Mass Stars
- Hot H2O Emission and Evidence for Turbulence in the Disk of a Young Star
- Identifying gaps in flaring Herbig Ae/Be disks using spatially resolved mid-infrared imaging. Are all group I disks transitional?
- X-Shooter study of accretion in Chamaeleon I
- Radiative transfer models of mid-infrared H2O lines in the Planet-forming Region of Circumstellar Disks
- Organic Molecules and Water in the Inner Disks of T Tauri Stars
- Tracing Slow Winds from T Tauri Stars via Low Velocity Forbidden Line Emission
- VLT-CRIRES Survey of Rovibrational CO Emission from Protoplanetary Disks
- Measuring Protoplanetary Disk Accretion with H I Pf-beta
- CO rovibrational emission as a probe of inner disk structure
- On the Transitional Disk Class: Linking Observations of T Tauri Stars & Physical Disk Models
- Non-stationary dynamo & magnetospheric accretion processes of the classical T Tauri star V2129 Oph
- DIGIT survey of far-infrared lines from protoplanetary disks I
- Evidence for a Snow Line Beyond the Transitional Radius in the TW Hya Protoplanetary Disk
- The Atomic and Molecular Content of Disks Around Very Low-mass Stars and Brown Dwarfs
- Single peaked CO emission line profiles from the inner regions of protoplanetary disks
- The structure of disks around intermediate-mass young stars from mid-infrared interferometry. Evidence for a population of group II disks with gaps
- Spitzer Spectroscopy of the Transition Object TW Hya
- The 2008 extreme outburst of the young eruptive variable star Ex Lupi
- Spectrally resolved pure rotational lines of water in protoplanetary disks
- Formation of Organic Molecules and Water in Warm Disk Atmospheres
- Accretion dynamics in the classical T Tauri star V2129 Oph
- An empirical sequence of disk gap opening revealed by rovibrational CO
- Probing stellar accretion with mid-infrared hydrogen lines
- Water depletion in the disk atmosphere of Herbig AeBe stars
- Radiation thermo-chemical models of protoplanetary discs. IV Modelling CO ro-vibrational emission from Herbig Ae discs
- The origin and evolution of transition discs: successes, problems and open questions
- First Detection of Near-Infrared Line Emission from Organics in Young Circumstellar Disks
- Ex Lupi from Quiescence to Outburst: Exploring the LTE Approach in Modelling Blended H2O and OH Mid-Infrared Emission
- Detection of warm water vapour in Taurus protoplanetary discs by Herschel
- Optical spectroscopy of EX Lupi during quiescence and outburst: Infall, wind, and dynamics in the accretion flow
- Measurements of water surface snow lines in classical protoplanetary disks
- The structure of disks around Herbig Ae/Be stars as traced by CO ro-vibrational emission
- Disks and Outflows in CO Rovibrational Emission from Embedded, Low-Mass Young Stellar Objects
- Discovery of OH in Circumstellar Disks Around Young Intermediate-Mass Stars
- Warm H2O and OH in the disk around the Herbig star HD 163296
- Understanding the water emission in the mid- and far-IR from protoplanetary disks around T~Tauri stars
- Candidate Water Vapor Lines to Locate the HO Snowline through High-Dispersion Spectroscopic Observations I. The Case of a T Tauri Star
- Depletion of molecular gas by an accretion outburst in a protoplanetary disk
- Mid-IR spectra of Pre-Main Sequence Herbig stars: an explanation for the non-detections of water lines
- Herschel-PACS observations of far-IR lines in YSOs I: [OI] and H2O at 63 microns
- The Evolution of Inner Disk Gas in Transition Disks
- A UV-to-MIR monitoring of DR Tau: exploring how water vapor in the planet formation region of the disk is affected by stellar accretion variability
- Detection of water vapor in the terrestrial planet forming region of a transition disk
- A proposed new diagnostic for Herbig disc geometry: FWHM versus J of CO ro-vibrational lines
- Herschel -PACS observations of [OI] and H2O in Cha II
- A Study of Ro-vibrational OH Emission from Herbig Ae/Be Stars
Cited by in corpus (45)
- Molecules with ALMA at Planet-forming Scales (MAPS) I: Program Overview and Highlights
- Water in star-forming regions (WISH): Physics and chemistry from clouds to disks as probed by Herschel spectroscopy
- Kinematic links and the co-evolution of MHD winds, jets, and inner disks from a high-resolution optical [OI] survey
- Hints for icy pebble migration feeding an oxygen-rich chemistry in the inner planet-forming region of disks
- Survey of cold water lines in protoplanetary disks: indications of systematic volatile depletion
- Evolution of protoplanetary disks from their taxonomy in scattered light: Group I vs. Group II
- CO2 infrared emission as a diagnostic of planet-forming regions of disks
- The Evolution of Disk Winds from a Combined Study of Optical and Infrared Forbidden Lines
- Modelling mid-infrared molecular emission lines from T Tauri stars
- MINDS. Abundant water and varying C/O across the disk of Sz 98 as seen by JWST/MIRI
- Scanning disk rings and winds in CO at 0.01-10 au: a high-resolution -band spectroscopy survey with IRTF-iSHELL
- The chemistry of disks around T Tauri and Herbig Ae/Be stars
- Chemically tracing the water snowline in protoplanetary disks with HCO
- The Chemical Inventory of the Inner Regions of Planet-forming Disks -- The JWST/MINDS Program
- The kinematics and excitation of infrared water vapor emission from planet-forming disks: results from spectrally-resolved surveys and guidelines for JWST spectra
- Candidate Water Vapor Lines to Locate the HO Snowline through High-Dispersion Spectroscopic Observations II. The Case of a Herbig Ae Star
- JWST Observations of Young protoStars (JOYS): overview of program and early results
- The ODYSSEUS Survey. Motivation and First Results: Accretion, Ejection, and Disk Irradiation of CVSO 109
- Herbig Stars: A Quarter Century of Progress
- Dust continuum emission and the upper limit fluxes of sub-millimeter water lines of the protoplanetary disk around HD 163296 observed by ALMA
- Observing the linked depletion of dust and CO gas at 0.1-10 au in disks of intermediate-mass stars
- A high resolution mid-infrared survey of water emission from protoplanetary disks
- Consistent dust and gas models for protoplanetary disks IV. A panchromatic view of protoplanetary disks
- Chemical Evolution in a Protoplanetary Disk within Planet Carved Gaps and Dust Rings
- The 1600 Angstrom Emission Bump in Protoplanetary Disks: A Spectral Signature of HO Dissociation
- The dry and carbon poor inner disk of TW Hya: evidence for a massive icy dust trap
- Probing planet formation and disk substructures in the inner disk of Herbig Ae stars with CO rovibrational emission
- OH mid-infrared emission as a diagnostic of HO UV photodissociation. III. Application to planet-forming disks
- Candidate Water Vapor Lines to Locate the Snowline through High-dispersion Spectroscopic Observations. III. Submillimeter and Lines
- A UV-to-NIR Study of Molecular Gas in the Dust Cavity Around RY Lupi
- HO distribution in the disc of HD 100546 and HD 163296: the role of dust dynamics and planet--disc interaction
- CLIcK: a Continuum and Line fItting Kit for circumstellar disks
- Reimagining the water snowline
- A model exploration of NIR ro-vibrational CO emission as a tracer of inner cavities in protoplanetary disks
- XUE. JWST spectroscopy of externally irradiated disks around young intermediate-mass stars
- Water and OH Emission from the inner disk of a Herbig Ae/Be star
- An unusual reservoir of water emission in the VV CrA A protoplanetary disk
- Gas kinematics of key prebiotic molecules in GV Tau N revealed with an ALMA, PdBI, and Herschel synergy
- Water vapor emission at the warm cavity wall of the HD 100546 disk as revealed by ALMA
- Evidence of a Disk-wind Origin for Fluorescent H in Classical T Tauri Stars
- Molecules with ALMA at Planet-forming Scales (MAPS). XV. Tracing protoplanetary disk structure within 20 au
- How leaky? A large parameter study of leaky dust traps to quantify the transport of pebbles and ice in protoplanetary discs
- The formation of planetary systems with SPICA
- Molecular Similarity and Water Diversity in Coeval Binary Disks: JWST/MIRI Observations of Sz 65 and Sz 66
- Linking Outer Disk Pebble Dynamics and Gaps to Inner Disk Water Enrichment