TOI-1670 b and c: An Inner Sub-Neptune with an Outer Warm Jupiter Unlikely to Have Originated from High-eccentricity Migration (2022)
Attributed to:
Astrophysics Consolidated Grant 2019-22
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.3847/1538-3881/ac5c4f
Publication URI: http://dx.doi.org/10.3847/1538-3881/ac5c4f
Type: Journal Article/Review
Parent Publication: The Astronomical Journal
Issue: 5