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Computer Generated Realistic Interstellar Icy Grain Models: Physicochemical Properties and Interaction with NH(3)

[Image: see text] Interstellar grains are composed by a rocky core (usually amorphous silicates) covered by an icy mantle, the most abundant molecule being H(2)O followed by CO, CO(2), NH(3), and also radicals in minor quantities. In dense molecular clouds, gas-phase chemical species freeze onto the...

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Detalles Bibliográficos
Autores principales: Germain, Aurèle, Tinacci, Lorenzo, Pantaleone, Stefano, Ceccarelli, Cecilia, Ugliengo, Piero
Formato: Online Artículo Texto
Lenguaje:English
Publicado: American Chemical Society 2022
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC9125691/
https://www.ncbi.nlm.nih.gov/pubmed/35620318
http://dx.doi.org/10.1021/acsearthspacechem.2c00004