Is there any linkage between interstellar aldehyde and alcohol?
arXiv:2108.06240 · doi:10.3847/1538-4357/ac1f31
Abstract
It is speculated that there might be some linkage between interstellar aldehydes and their corresponding alcohols. Here, an observational study and astrochemical modeling are coupled together to illustrate the connection between them. The ALMA Cycle 4 data of a hot molecular core, G10.47+0.03 is utilized for this study. Various aldehydes (acetaldehyde, propanal, and glycolaldehyde), alcohols (methanol and ethylene glycol), and a ketone (acetone) are identified in this source. The excitation temperatures and the column densities of these species were derived via the rotation diagram method assuming LTE conditions. An extensive investigation is carried out to understand the formation of these species. Six pairs of aldehyde-alcohol: i) methanal and methanol; ii) ethanal and ethanol; iii) propanal and 1-propanol; iv) propenal and allyl alcohol; v) propynal and propargyl alcohol; vi) glycolaldehyde and ethylene glycol; vii) along with one pair of ketone-alcohol (acetone and isopropanol) and viii) ketene-alcohol (ethenone and vinyl alcohol) are considered for this study. Two successive hydrogenation reactions in the ice phase are examined to form these alcohols from aldehydes, ketone, and ketene, respectively. Quantum chemical methods are extensively executed to review the ice phase formation route and the kinetics of these species. Based on the obtained kinetic data, astrochemical modeling is employed to derive the abundances of these aldehydes, alcohols, ketone, and ketene in this source. It is seen that our model could successfully explain the observed abundances of various species in this hot molecular core.
arXiv comment34 pages, 11 figures, Accepted for the publication in the Astrophysical Journal
References in corpus (61)
- The UMIST database for astrochemistry 2012
- Complex Chemistry in Star-Forming Regions: An Expanded Gas-Grain Warm-up Chemical Model
- Formation of methyl formate and other organic species in the warm-up phase of hot molecular cores
- The Cologne Database for Molecular Spectroscopy, CDMS, in the Virtual Atomic and Molecular Data Centre, VAMDC
- Formation rates of complex organics in UV irradiated CH3OH-rich ices I: Experiments
- Non-thermal desorption from interstellar dust grains via exothermic surface reactions
- Complex organic molecules in the interstellar medium: IRAM 30 m line survey of Sagittarius B2(N) and (M)
- 2018 Census of Interstellar, Circumstellar, Extragalactic, Protoplanetary Disk, and Exoplanetary Molecules
- Polycylcic Aromatic Hydrocarbons (PAH's) in dense cloud chemistry
- On the Formation of CO2 and Other Interstellar Ices
- Reaction Networks For Interstellar Chemical Modelling: Improvements and Challenges
- Detection of a branched alkyl molecule in the interstellar medium: iso-propyl cyanide
- Binding energies: new values and impact on the efficiency of chemical desorption
- H-atom addition and abstraction reactions in mixed CO, H2CO and CH3OH ices: an extended view on complex organic molecule formation
- Experimental evidence for Glycolaldehyde and Ethylene Glycol formation by surface hydrogenation of CO molecules under dense molecular cloud conditions
- An interferometric study of the low-mass protostar IRAS 16293-2422: small scale organic chemistry
- First detection of glycolaldehyde outside the Galactic Center
- Complex organic molecules in comets C/2012 F6 (Lemmon) and C/2013 R1 (Lovejoy): detection of ethylene glycol and formamide
- The formation of ethylene glycol and other complex organic molecules in star-forming regions
- Organic Molecules in the Galactic Center. Hot Core Chemistry without Hot Cores
- Formation of Glycerol through Hydrogenation of CO ice under Prestellar Core Conditions
- Detection of abundant solid methanol toward young low mass stars
- First results from the CALYPSO IRAM-PdBI survey. II. Resolving the hot corino in the Class 0 protostar NGC 1333-IRAS2A
- Trigonometric parallaxes to star-forming regions within 4 kpc of the galactic center
- H-atom bombardment of CO2, HCOOH and CH3CHO containing ices
- Glycolaldehyde Formation via the Dimerisation of the Formyl Radical
- An Approach to Estimate the Binding energy of Interstellar Species
- The ALMA-PILS survey: Formaldehyde deuteration in warm gas on small scales toward IRAS 16293-2422 B
- STATCONT: A statistical continuum level determination method for line-rich sources
- Parameterizing the interstellar dust temperature
- Antifreeze in the hot core of Orion - First detection of ethylene glycol in Orion-KL
- Searching for Trans Ethyl Methyl Ether in Orion KL
- Identification of pre-biotic molecules containing Peptide-like bond in a hot molecular core, G10.47+0.03
- Sticking coefficient of hydrogen and deuterium on silicates under interstellar conditions
- Hydrogen transfer reactions of interstellar Complex Organic Molecules
- Search for Interstellar monohydric Thiols
- Structure of the hot molecular core G10.47+0.03
- Formation of interstellar propanal and 1-propanol ice: a pathway involving solid-state CO hydrogenation
- Formation of water and methanol in star forming molecular clouds
- Composition and evolution of Interstellar Grain mantle under the effects of photo-dissociation
- High-velocity gas toward hot molecular cores: evidence for collimated outflows from embedded sources
- Chemical modeling for predicting the abundances of certain aldimines and amines in hot cores
- A New and Simple Approach to Determine the Abundance of Hydrogen Molecules on Interstellar Ice Mantles
- Tunneling Rate Constants for H2CO+H on Amorphous Solid Water Surfaces
- Effects of Initial Condition and Cloud Density on the Composition of the Grain Mantle
- Methyl Acetate and its singly deuterated isotopomers in the interstellar medium
- Effective grain surface area in the formation of molecular hydrogen in interstellar clouds
- Deuterium enrichment of the interstellar grain mantle
- Deuterium Enrichment of the Interstellar Medium
- Chemical modelling of glycolaldehyde and ethylene glycol in star-forming regions
- Time evolution of simple molecules during proto-star collapse
- Chemistry and physics of a low-metallicity hot core in the Large Magellanic Cloud
- Chemical complexity of phosphorous bearing species in various regions of the Interstellar medium
- Isomerization and Decomposition Reactions of Acetaldehyde Relevant to Atmospheric Processes from Dynamics Simulations on Neural Network-Based Potential Energy Surfaces
- Identification of Methyl Isocyanate and Other Complex Organic Molecules in a Hot Molecular Core, G31.41+0.31
- Chemical and radiative transfer modeling of Propylene Oxide
- The Possibility of Forming Propargyl Alcohol in the Interstellar Medium
- Tracing the atomic nitrogen abundance in star-forming regions with ammonia deuteration
- Effect of binding energies on the encounter desorption
- Tunnelling dominates the reactions of hydrogen atoms with unsaturated alcohols and aldehydes in the dense medium
- On the Encounter Desorption of Hydrogen Atoms on Ice Mantle
Cited by in corpus (9)
- Identification of interstellar amino acetonitrile in the hot molecular core G10.47+0.03: Possible glycine survey candidate for the future
- Enhanced formation of interstellar complex organic molecules on carbon monoxide ice
- Identification of the simplest sugar-like molecule glycolaldehyde towards the hot molecular core G358.93-0.03 MM1
- Assessing realistic binding energies of some essential interstellar radicals with amorphous solid water. A fully quantum chemical approach
- Detection of complex nitrogen-bearing molecule ethyl cyanide towards the hot molecular core G10.47+0.03
- Detection of antifreeze molecule ethylene glycol in the hot molecular core G358.930.03 MM1
- Hydrogenation of acetaldehyde on interstellar ice analogs reveals limited destruction
- Study of Complex Nitrogen and Oxygen-bearing Molecules toward the High-mass Protostar IRAS 180891732
- Metallic species in interstellar medium: Astrochemical modeling