Revising Properties of Planet–Host Binary Systems. IV. The Radius Distribution of Small Planets in Binary Star Systems Is Dependent on Stellar Separation

Small planets ( R _p ≤ 4 R _⊕ ) are divided into rocky super-Earths and gaseous sub-Neptunes separated by a radius gap, but the mechanisms that produce these distinct planet populations remain unclear. Binary stars are the only main-sequence systems with an observable record of the protoplanetary di...

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Ngā taipitopito rārangi puna kōrero

Ngā kaituhi matua:	Kendall Sullivan, Adam L. Kraus, Travis A. Berger, Trent J. Dupuy, Elise Evans, Eric Gaidos, Daniel Huber, Michael J. Ireland, Andrew W. Mann, Erik A. Petigura, Pa Chia Thao, Mackenna L. Wood, Jingwen Zhang
Hōputu:	Artigo
Reo:	Inglês
I whakaputaina:	IOP Publishing 2024-01-01
Rangatū:	The Astronomical Journal
Ngā marau:	Binary stars Super Earths Exoplanets Mini Neptunes Exoplanet formation Planet hosting stars
Urunga tuihono:	https://doi.org/10.3847/1538-3881/ad6310
Ngā Tūtohu:	Tāpirihia he Tūtohu Kāore He Tūtohu, Me noho koe te mea tuatahi ki te tūtohu i tēnei pūkete!