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TOI-1670 b and c: An Inner Sub-Neptune with an Outer Warm Jupiter Unlikely to Have Originated from High-eccentricity Migration (2022)

First Author: Tran Q

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