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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...
| Autores principales: | , , , , , |
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| Formato: | Online Artículo Texto |
| Lenguaje: | English |
| Publicado: |
MDPI
2014
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| Materias: | |
| 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 |