Disk Evolution, Element Abundances and Cloud Properties of Young Gas Giant Planets

We discuss the chemical pre-conditions for planet formation, in terms of gas and ice abundances in a protoplanetary disk, as function of time and position, and the resulting chemical composition and cloud properties in the atmosphere when young gas giant planets form, in particular discussing the ef...

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Detalles Bibliográficos
Autores principales: Helling, Christiane, Woitke, Peter, Rimmer, Paul B., Kamp, Inga, Thi, Wing-Fai, Meijerink, Rowin
Formato: Online Artículo Texto
Lenguaje:English
Publicado: MDPI 2014
Materias:
Article
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC4187161/
https://www.ncbi.nlm.nih.gov/pubmed/25370190
http://dx.doi.org/10.3390/life4020142

Internet

https://www.ncbi.nlm.nih.gov/pmc/articles/PMC4187161/
https://www.ncbi.nlm.nih.gov/pubmed/25370190
http://dx.doi.org/10.3390/life4020142

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