Symmetric Atom–Atom and Ion–Atom Processes in Stellar Atmospheres

Symmetric Atom–Atom and Ion–Atom Processes in Stellar Atmospheres

We present the results of the influence of two groups of collisional processes (atom–atom and ion–atom) on the optical and kinetic properties of weakly ionized stellar atmospheres layers. The first type includes radiative processes of the photodissociation/association and radiative charge exchange,...

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Detalles Bibliográficos
Autores principales: Vladimir A. Srećković, Ljubinko M. Ignjatović, Milan S. Dimitrijević
Formato: Artículo
Lenguaje:English
Publicado: MDPI AG 2017-12-01
Colección:Atoms
Materias:
atomic processes
molecular processes
radiative transfer
absorption quasi-molecular bands
sun:atmosphere
sun:photosphere
stars:atmospheres
white dwarfs
Acceso en línea:https://www.mdpi.com/2218-2004/6/1/1

Internet

https://www.mdpi.com/2218-2004/6/1/1

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