Formation of the Methyl Cation by Photochemistry in a Protoplanetary Disk
arXiv:2401.03296 · doi:10.1038/s41586-023-06307-x
Abstract
Forty years ago it was proposed that gas phase organic chemistry in the interstellar medium was initiated by the methyl cation CH3+, but hitherto it has not been observed outside the Solar System. Alternative routes involving processes on grain surfaces have been invoked. Here we report JWST observations of CH3+ in a protoplanetary disk in the Orion star forming region. We find that gas-phase organic chemistry is activated by UV irradiation.
Published in Nature
References in corpus (13)
- The distance to the Orion Nebula
- JWST MIRI flight performance: The Medium-Resolution Spectrometer
- The chemistry and spatial distribution of small hydrocarbons in UV-irradiated molecular clouds: the Orion Bar PDR
- The full infrared spectrum of molecular hydrogen
- MINDS. The detection of CO with JWST-MIRI indicates abundant CO in a protoplanetary disk
- The penetration of FUV radiation into molecular clouds
- PDRs4All: A JWST Early Release Science Program on radiative feedback from massive stars
- OH mid-infrared emission as a diagnostic of HO UV photodissociation. I. Model and application to the HH 211 shock
- Molecular line emission from a protoplanetary disk irradiated externally by a nearby massive star
- The PhotoDissociation Region Toolbox: Software and Models for Astrophysical Analysis
- Contribution of polycyclic aromatic hydrocarbon ionization to neutral gas heating in galaxies: model versus observations
- OH mid-infrared emission as a diagnostic of HO UV photodissociation. II. Application to interstellar PDRs
- Wavelength Calibration and Resolving Power of the JWST MIRI Medium Resolution Spectrometer
Cited by in corpus (21)
- PDRs4All III: JWST's NIR spectroscopic view of the Orion Bar
- OH mid-infrared emission as a diagnostic of HO UV photodissociation. III. Application to planet-forming disks
- Sub-Doppler optical-optical double-resonance spectroscopy using a cavity-enhanced frequency comb probe
- PDRs4All XI. Detection of infrared CH and CH rovibrational emission in the Orion Bar and disk d203-506: evidence of chemical pumping
- A Novel Method to Estimate the FUV Flux and a Catalogue for Star-Hosting Discs in Nearby Star-Forming Regions
- PDRs4All. X. ALMA and JWST detection of neutral carbon in the externally irradiated disk d203-506: Undepleted gas-phase carbon
- PDRs4All. XII. FUV-driven formation of hydrocarbon radicals and their relation with PAHs
- PDRs4All VII. The 3.3 m aromatic infrared band as a tracer of physical properties of the ISM in galaxies
- A tell-tale tracer for externally irradiated protoplanetary disks: comparing the [CI] 8727 A line and ALMA observations in proplyds
- XUE. JWST spectroscopy of externally irradiated disks around young intermediate-mass stars
- Externally irradiated young stars in NGC 3603. A JWST NIRSpec catalogue of pre-main-sequence stars in a massive star formation region
- Tracking the Chemical Evolution of Hydrocarbons Through Carbon Grain Supply in Protoplanetary Disks
- PDRs4All XV: CH radical and H molecular ion in the irradiated protoplanetary disk d203-506
- PDRs4All: XVIII. The evolution of the PAH ionisation and PAH size distribution across the Orion Bar
- H3+ in irradiated protoplanetary disks: Linking far-ultraviolet radiation and water vapor
- Line ratio identification of external photoevaporation
- High-resolution ro-vibrational and rotational spectroscopy of the open-shell, linear CCH ion ()
- Spatial distribution of organics in the Horsehead nebula: Signposts of chemistry driven by atomic carbon
- Detection of CO ice in the planetary nebula NGC 6302
- Acenaphthene Derivatives as Signatures of CH Reactivity with Methylated Naphthalenes
- PDRs4All XVIII. JWST-NIRCam Photometric properties of protoplanetary disks in the Orion Nebula Cluster