TESS Giants Transiting Giants. IV. A Low-density Hot Neptune Orbiting a Red Giant Star
Hot Neptunes, gaseous planets smaller than Saturn (∼3–8 R _⊕ ) with orbital periods less than 10 days, are rare. Models predict this is due to high-energy stellar irradiation stripping planetary atmospheres over time, often leaving behind only rocky planetary cores. Using our TESS full-frame-image p...
Wedi'i Gadw mewn:
| Prif Awduron: | , , , , , , , , , , , , , , , , |
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| Fformat: | Artigo |
| Iaith: | Inglês |
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IOP Publishing
2024-01-01
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| Cyfres: | The Astronomical Journal |
| Pynciau: | |
| Mynediad Ar-lein: | https://doi.org/10.3847/1538-3881/ad4149 |
| Tagiau: |
Dim Tagiau, Byddwch y cyntaf i dagio'r cofnod hwn!
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