ON THE COMPOSITION OF YOUNG, DIRECTLY IMAGED GIANT PLANETS

The past decade has seen significant progress on the direct detection and characterization of young, self-luminous giant planets at wide orbital separations from their host stars. Some of these planets show evidence for disequilibrium processes like transport-induced quenching in their atmospheres;...

Deskribapen osoa

Gorde:
Xehetasun bibliografikoak
Argitaratua izan da:Astrophys J
Egile Nagusiak: Moses, J. I., Marley, M. S., Zahnle, K., Line, M. R., Fortney, J. J., Barman, T. S., Visscher, C., Lewis, N. K., Wolff, M. J.
Formatua: Artigo
Hizkuntza:Inglês
Argitaratua: 2016
Gaiak:
Article
Sarrera elektronikoa:https://ncbi.nlm.nih.gov/pmc/articles/PMC6547835/
https://ncbi.nlm.nih.gov/pubmed/31171882
https://ncbi.nlm.nih.govhttp://dx.doi.org/10.3847/0004-637X/829/2/66
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