1 code implementation • 13 Sep 2019 • Hsiang-Chih Hwang, Nadia Zakamska
Instead, our best-fit models suggest that the formation of these short-period binaries is delayed by 0. 6-3 Gyr, and the disappearing time is less than the age of the thick disk.
Solar and Stellar Astrophysics Astrophysics of Galaxies
