[astro-ph.GA] Polycyclic aromatic hydrocarbons (PAHs) are ubiquitous in the interstellar medium and are among its smallest carbonaceous grains.
photodissociation
Searching For The Elusive CH2+ With The James Webb Space Telescope. Another Carbocation To Constrain Astrochemical Networks
[astro-ph.GA] Carbocations are key species in interstellar chemistry, providing entry points for building larger hydrocarbons. CH+, and more recently, CH3+, have been detected. Other carbocations await detection to provide a […]
CO and N2 Produced from H2O, CO2, and NH3 Cometary Ice Analogs
Hypervolatile species such as carbon monoxide (CO) and molecular nitrogen (N2) have been detected in comets, and could be used to constrain comet formation temperature conditions if their presence is […]
The Response of Planetary Atmospheres To The Impact Of Icy Comets II: Exo-Earth Analogues
The orbital regime of a terrestrial planet plays a significant role in shaping its atmospheric dynamics, climate, and hence potential habitability.
Re-analysis of 10 Hot-Jupiter Atmospheres With Disequilibrium Chemistry Retrieval
Constraining the chemical structure of exoplanetary atmospheres is pivotal for interpreting spectroscopic data and understanding planetary evolution.
OH Mid-infrared Emission as a Diagnostic of H2O UV Photodissociation. III. Application to Planet-forming Disks
JWST gives a unique access to the physical and chemical structure of inner disks (<10~au), where the majority of the planets are forming. However, the interpretation of mid-infrared (mid-IR) spectra […]
