Quantifying the Effect of Short-timescale Stellar Activity Upon Transit Detection in M Dwarfs
M dwarf stars comprise 70%–80% of the galaxy's stars and host most of its rocky planets. They also differ from Sunlike stars in that they are “active” for billions of years or more: rotating quickly, flaring often, and emitting large amounts of UV and X-ray light. The effects of stellar activity upo...
Kaydedildi:
| Asıl Yazarlar: | , , , |
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| Materyal Türü: | Artigo |
| Dil: | Inglês |
| Baskı/Yayın Bilgisi: |
IOP Publishing
2025-01-01
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| Seri Bilgileri: | The Astronomical Journal |
| Konular: | |
| Online Erişim: | https://doi.org/10.3847/1538-3881/ada898 |
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