X-ray photodesorption of complex organic molecules in protoplanetary disks -- I. Acetonitrile CH3CN
arXiv:2306.13048 · doi:10.1051/0004-6361/202346209
Abstract
X-rays emitted from pre-main-sequence stars at the center of protoplanetary disks can induce nonthermal desorption from interstellar ices populating the cold regions. This X-ray photodesorption needs to be quantified for complex organic molecules (COMs), including acetonitrile CH3CN, which has been detected in several disks. We experimentally estimate the X-ray photodesorption yields of neutral species from pure CH3CN ices and from interstellar ice analogs for which CH3CN is mixed either in a CO- or H2O-dominated ice. The ices were irradiated at 15 K by soft X-rays (400-600 eV) from synchrotron light (SOLEIL synchrotron). X-ray photodesorption was probed in the gas phase via quadrupole mass spectrometry. X-ray photodesorption yields were derived from the mass signals and were extrapolated to higher X-ray energies for astrochemical models. X-ray photodesorption of the intact CH3CN is detected from pure CH3CN ices and from mixed 13CO:CH3CN ices, with a yield of about 5x10^(-4) molecules/photon at 560 eV. When mixed in H2O-dominated ices, X-ray photodesorption of the intact CH3CN at 560 eV is below its detection limit, which is 10^(-4) molecules/photon. Yields associated with the desorption of HCN, CH4 , and CH3 are also provided. The derived astrophysical yields significantly depend on the local conditions expected in protoplanetary disks. They vary from 10^(-4) to 10(-6) molecules/photon for the X-ray photodesorption of intact CH3CN from CO-dominated ices. Only upper limits varying from 5x10^(-5) to 5x10^(-7) molecules/photon could be derived for the X-ray photodesorption of intact CH3CN from H2O-dominated ices. X-ray photodesorption of intact CH3CN from interstellar ices might in part explain the abundances of CH3CN observed in protoplanetary disks. The desorption efficiency is expected to vary with the local physical conditions, hence with the disk region.
References in corpus (19)
- X-Ray Spectroscopy of Stars
- The cometary composition of a protoplanetary disk as revealed by complex cyanides
- Molecular Hydrogen Emission from Protoplanetary Disks II. Effects of X-ray Irradiation and Dust Evolution
- UV photodesorption of methanol in pure and CO-rich ices: desorption rates of the intact molecule and of the photofragments
- A Survey of CH3CN and HC3N in Protoplanetary Disks
- The Distribution and Excitation of CHCN in a Solar Nebula Analog
- Auger Electron Cascades in Water and Ice
- Photoelectric cross-sections of gas and dust in protoplanetary disks
- X-ray photodesorption from water ice in protoplanetary disks and X-ray dominated regions
- X-ray induced chemistry of water and related molecules in low-mass protostellar envelopes
- Nitrile versus isonitrile adsorption at interstellar grains surfaces: I - Hydroxylated surfaces
- X-ray emission processes in stars
- Complex organic molecules in protoplanetary disks : X-ray photodesorption from methanol-containing ices. Part I -- Pure methanol ices
- Photo-desorption of H2O:CO:NH3 circumstellar ice analogs: Gas-phase enrichment
- Photodesorption of acetonitrile CH3CN in UV-irradiated regions of the Interstellar Medium: an experimental evidence
- Complex organic molecules in protoplanetary disks: X-ray photodesorption from methanol-containing ices. Part II -- Mixed methanol-CO and methanol-H2O ices
- X-ray induced desorption and photochemistry in CO ice
- Desorption of neutrals, cations and anions from core-excited amorphous solid water
- Indirect X-ray photodesorption of 15N2 and 13CO from mixed and layered ices