Faraday Discuss., 2023, 245,586-608
DOI: 10.1039/D3FD00039G, Paper
DOI: 10.1039/D3FD00039G, Paper
Open Access
This article is licensed under a Creative Commons Attribution 3.0 Unported Licence.Marie Van de Sande, Catherine Walsh, Tom J. Millar
The first AGB chemical kinetics model that includes porosity, dust–gas chemistry and companion UV photons, allows us to unravel the interplay of the complexities and identify suites of molecules to determine the presence of a companion star.
The content of this RSS Feed (c) The Royal Society of Chemistry
The first AGB chemical kinetics model that includes porosity, dust–gas chemistry and companion UV photons, allows us to unravel the interplay of the complexities and identify suites of molecules to determine the presence of a companion star.
The content of this RSS Feed (c) The Royal Society of Chemistry