MINDS. Abundant water and varying C/O across the disk of Sz 98 as seen by JWST/MIRI
arXiv:2307.09301 · doi:10.1051/0004-6361/202347005
Abstract
MIRI/MRS on board the JWST allows us to probe the inner regions of protoplanetary disks. Here we examine the disk around the classical T Tauri star Sz 98, which has an unusually large dust disk in the millimetre with a compact core. We focus on the HO emission through both its ro-vibrational and pure rotational emission. Furthermore, we compare our chemical findings with those obtained for the outer disk from Atacama Large Millimeter/submillimeter Array (ALMA) observations. In order to model the molecular features in the spectrum, the continuum was subtracted and LTE slab models were fitted. The spectrum was divided into different wavelength regions corresponding to HO lines of different excitation conditions, and the slab model fits were performed individually per region. We confidently detect CO, HO, OH, CO, and HCN in the emitting layers. The isotopologue HO is not detected. Additionally, no other organics, including CH, are detected. This indicates that the C/O ratio could be substantially below unity, in contrast with the outer disk. The HO emission traces a large radial disk surface region, as evidenced by the gradually changing excitation temperatures and emitting radii. The OH and CO emission are relatively weak. It is likely that HO is not significantly photodissociated; either due to self-shielding against the stellar irradiation, or UV-shielding from small dust particles. The relative emitting strength of the different identified molecular features point towards UV-shielding of HO in the inner disk of Sz 98, with a thin layer of OH on top. The majority of the organic molecules are either hidden below the dust continuum, or not present. In general, the inferred composition points to a sub-solar C/O ratio (<0.5) in the inner disk, in contrast with the larger than unity C/O ratio in the gas in the outer disk found with ALMA.
Updated to accepted version. Accepted by A&A on September 23 2023. 18 pages, 11 figures
References in corpus (36)
- The Gaia mission
- Gaia Data Release 3: Summary of the content and survey properties
- X-Shooter spectroscopy of young stellar objects in Lupus: Accretion properties of class II and transitional objects
- The Science Performance of JWST as Characterized in Commissioning
- Astrochemistry and compositions of planetary systems
- JWST MIRI flight performance: The Medium-Resolution Spectrometer
- Water in star-forming regions (WISH): Physics and chemistry from clouds to disks as probed by Herschel spectroscopy
- The Spitzer c2d Survey of Large, Nearby, Interstellar Clouds. XI. Lupus Observed With IRAC and MIPS
- Protoplanetary disk rings and gaps across ages and luminosities
- Physical properties of dusty protoplanetary disks in Lupus: evidence for viscous evolution?
- Mapping accretion and its variability in the young open cluster NGC 2264: a study based on u-band photometry
- Formation of Water in the Warm Atmospheres of Protoplanetary Disks
- MINDS. The detection of CO with JWST-MIRI indicates abundant CO in a protoplanetary disk
- Connection between jets, winds and accretion in T Tauri stars: the X-shooter view
- Hints for icy pebble migration feeding an oxygen-rich chemistry in the inner planet-forming region of disks
- Water in the terrestrial planet-forming zone of the PDS 70 disk
- Investigating grain growth in disks around southern T Tauri stars at millimetre wavelengths
- CSI 2264: Characterizing Young Stars in NGC 2264 with Short-Duration, Periodic Flux Dips in their Light Curves
- Probing stellar accretion with mid-infrared hydrogen lines
- The depletion of water during dispersal of planet-forming disk regions
- Scanning disk rings and winds in CO at 0.01-10 au: a high-resolution -band spectroscopy survey with IRTF-iSHELL
- OH mid-infrared emission as a diagnostic of HO UV photodissociation. I. Model and application to the HH 211 shock
- JWST MIRI/MRS in-flight absolute flux calibration and tailored fringe correction for unresolved sources
- The kinematics and excitation of infrared water vapor emission from planet-forming disks: results from spectrally-resolved surveys and guidelines for JWST spectra
- JWST/MIRI Spectroscopy of the Disk of the Young Eruptive Star EX Lup in Quiescence
- Observing Carbon & Oxygen Carriers in Protoplanetary Disks at Mid-infrared Wavelengths
- A blue depression in the optical spectra of M dwarfs
- Tracing pebble drift and trapping using radial carbon depletion profiles in protoplanetary disks
- Chemical evolution in ices on drifting, planet-forming pebbles
- Water UV-shielding in the terrestrial planet-forming zone: Implications for carbon dioxide emission
- The ASAS-SN Catalog of Variable Stars VIII: "Dipper" Stars in the Lupus Star-Forming Region
- Water shielding in the terrestrial planet-forming zone: Implication for inner disk organics
- Water UV-Shielding in the Terrestrial Planet-Forming Zone: Implications for Oxygen-18 Isotope Anomalies in H2-18O Infrared Emission and Meteorites
- The mid-IR water and silicate relation in protoplanetary disks
- Mid-infrared blends and continuum signatures of dust drift and accretion in protoplanetary disks
- An unusual reservoir of water emission in the VV CrA A protoplanetary disk
Cited by in corpus (27)
- JWST Observations of Young protoStars (JOYS): overview of program and early results
- Mind the gap: Distinguishing disc substructures and their impact on the inner disc composition
- JWST Observations of Young protoStars (JOYS). Overview of gaseous molecular emission and absorption in low-mass protostars
- Bayesian Analysis of Molecular Emission and Dust Continuum of Protoplanetary Disks
- MINDS. A multi-instrument investigation into the molecule-rich JWST-MIRI spectrum of the DF Tau binary system
- A high-resolution survey of protoplanetary disks in Lupus and the nature of compact disks
- CO2-rich protoplanetary discs as a probe of dust radial drift & trapping
- OH mid-infrared emission as a diagnostic of HO UV photodissociation. III. Application to planet-forming disks
- MINDS. JWST-MIRI reveals a peculiar CO-rich chemistry in the drift-dominated disk CX Tau
- MINDS: The very low-mass star and brown dwarf sample -- Hidden water in carbon-dominated protoplanetary disks
- Changing disc compositions via internal photoevaporation I: Solar-mass stars
- Chemical transformation of CO in evolving protoplanetary discs across stellar masses: a route to C-rich inner regions
- Understanding JWST water spectra: what can thermochemical models tell us about the (cold) water in protoplanetary disks?
- Radiative Nonideal MHD Simulations of Inner Protoplanetary Disks: Temperature Structures, Asymmetric Winds, and Episodic Surface Accretion
- Disentangling the dust and gas contributions of the JWST/MIRI spectrum of Sz28
- How external photo-evaporation changes the chemical composition of the inner disc
- XUE. JWST spectroscopy of externally irradiated disks around young intermediate-mass stars
- Extended source fringe flats for the JWST MIRI Medium Resolution Spectrometer
- Tracking the Chemical Evolution of Hydrocarbons Through Carbon Grain Supply in Protoplanetary Disks
- MINDS. Young binary systems with JWST/MIRI: Variable water-rich primaries and extended emission
- Changing disc compositions via internal photoevaporation II: M dwarf systems
- On the diversification and dissipation of protoplanetary disks
- Improving Accretion Diagnostics for Young Stellar Objects with Mid-infrared Hydrogen lines from JWST/MIRI
- Zooming into the water snowline: high resolution water observations of the HL Tau disk
- Inelastic Triatom-Atom Quantum Close-Coupling Dynamics in Full Dimensionality: all rovibrational mode quenching of water due to H impact on a six-dimensional potential energy surface
- Gaps and Rings: A Near-Universal Trait of Extended Protoplanetary Discs
- Molecular Similarity and Water Diversity in Coeval Binary Disks: JWST/MIRI Observations of Sz 65 and Sz 66