The white dwarf binary pathways sur v ey -X. Gaia orbits for known UV excess binaries
Date Issued
2024-03
Author(s) USM
DOI
10.1093/mnras/stae807
Abstract
White dwarfs with an F, G, or K type companion represent the last common ancestor for a plethora of exotic systems throughout the galaxy, though to this point very few of them have been fully characterized in terms of orbital period and component masses,
