Mid-to-late M Dwarfs Lack Jupiter Analogs

Cold Jovian planets play an important role in sculpting the dynamical environment in which inner terrestrial planets form. The core accretion model predicts that giant planets cannot form around low-mass M dwarfs, although this idea has been challenged by recent planet discoveries. Here, we investig...

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Principais autores:	Emily K. Pass, Jennifer G. Winters, David Charbonneau, Jonathan M. Irwin, David W. Latham, Perry Berlind, Michael L. Calkins, Gilbert A. Esquerdo, Jessica Mink
格式:	Artigo
語言:	Inglês
出版:	IOP Publishing 2023-01-01
叢編:	The Astronomical Journal
主題:	Extrasolar gaseous giant planets M dwarf stars Radial velocity Surveys High resolution spectroscopy
在線閱讀:	https://doi.org/10.3847/1538-3881/acd349
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