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Thermal escape from extrasolar giant planets
The detection of hot atomic hydrogen and heavy atoms and ions at high altitudes around close-in extrasolar giant planets (EGPs) such as HD209458b implies that these planets have hot and rapidly escaping atmospheres that extend to several planetary radii. These characteristics, however, cannot be gen...
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Main Authors: | , , , |
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Formato: | Artigo |
Idioma: | Inglês |
Publicado em: |
The Royal Society Publishing
2014
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Acesso em linha: | https://ncbi.nlm.nih.gov/pmc/articles/PMC3982429/ https://ncbi.nlm.nih.gov/pubmed/24664923 https://ncbi.nlm.nih.govhttp://dx.doi.org/10.1098/rsta.2013.0089 |
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