Atomic iron and titanium in the atmosphere of the exoplanet KELT-9b

To constrain the formation history of an exoplanet, we need to know its chemical composition1–3. With an equilibrium temperature of about 4,050 kelvin4, the exoplanet KELT-9b (also known as HD 195689b) is an archetype of the class of ultrahot Jupiters that straddle the transition between stars and g...

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Vydáno v:Nature
Hlavní autoři: Hoeijmakers, H. Jens, Ehrenreich, David, Heng, Kevin, Kitzmann, Daniel, Grimm, Simon L., Allart, Romain, Deitrick, Russell, Wyttenbach, Aurélien, Oreshenko, Maria, Pino, Lorenzo, Rimmer, Paul B., Molinari, Emilio, Di Fabrizio, Luca
Médium: Artigo
Jazyk:Inglês
Vydáno: 2018
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On-line přístup:https://ncbi.nlm.nih.gov/pmc/articles/PMC6322651/
https://ncbi.nlm.nih.gov/pubmed/30111838
https://ncbi.nlm.nih.govhttp://dx.doi.org/10.1038/s41586-018-0401-y
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