The DOI matches its Crossref record; 81 of the 81 references it cites were found in a registry or an index.
3D mixing in hot Jupiters atmospheres: I. Application to the day/night cold trap in HD 209458b⋆
Open accessAbstract
Context. Hot Jupiters exhibit atmospheric temperatures ranging from hundreds to thousands of Kelvin. Because of their large day-night temperature differences, condensable species that are stable in the gas phase on the dayside – such as TiO and silicates – may condense and gravitationally settle on the nightside. Atmospheric circulation may counterbalance this tendency to gravitationally settle. This three-dimensional (3D) mixing of condensable species has not previously been studied for hot Jupiters, yet it is crucial to assess the existence and distribution of TiO and silicates in the atmospheres of these planets.
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Cites
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Metadata
- Authors
- Parmentier, V., Showman, A. P., & Lian, Y.
- Venue
- Astronomy & Astrophysics
- Publisher
- EDP Sciences
- Published
- 2013-10
- Volume
- 558
- Pages
- A91
- ISSN
- 0004-6361 (ISSN-L)
- 1432-0746
- OpenAlex
- W4292406750
- Cited by
- 371
- References
- 81
- FWCI
- 13.49
- Type
- journal article
- Language
- en
- Open access
- bronze
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- Parmentier, V., Showman, A. P., & Lian, Y. (2013). 3D mixing in hot Jupiters atmospheres: I. Application to the day/night cold trap in HD 209458b⋆. Astronomy & Astrophysics. https://doi.org/10.1051/0004-6361/201321132
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