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Trapping (sub-)Neptunes similar to TOI-216b at the inner disk rim. Implications for the disk viscosity and the Neptunian desert
Type of publication: Article
Citation:
Publication status: Published
Journal: Astronomy & Astrophysics
Volume: 666
Year: 2022
Month: October
Pages: A63
ISSN: 0004-6361
URL: https://www.aanda.org/articles...
DOI: 10.1051/0004-6361/202244461
Userfields: eid={A63}, archiveprefix={arXiv}, eprint={2208.10257}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2022A&A...666A..63C}, adsnote={Provided by the SAO/NASA Astrophysics Data System},
Keywords: Astrophysics - Earth and Planetary Astrophysics, hydrodynamics, planet-disk interactions, planetary systems, planets and satellites: formation, protoplanetary disks
Authors Chrenko, O.
Chametla, R. O.
Nesvorný, D.
{Flock}, M.
Added by: [OCh]
Total mark: 0
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