Gas disk interactions, tides and relativistic effects in the rocky planet formation at the substellar mass limit

Context. The confirmed exoplanet population around very low mass stars is increasing considerable through data from the latest space missions and improvements in ground-based observations, particularly with the detection of Earth-like planets in the habitable zones. However, theoretical models need...

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Bibliographic Details

Main Author:	Sánchez, Mariana B. (author)
Other Authors:	de Elía, Gonzalo C. (author), Downes, José (author)
Format:	article
Language:	English
Published:	2022
Subjects:	Planets and satellites: terrestrial planets Planets and satellites: formation Stars: low-mass Planet-disk interactions Planet-star interactions Methods: numerical
Online Access:	https://hdl.handle.net/20.500.12008/39207
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