Close detached white dwarf + brown dwarf binaries: further evidence for low values of the common envelope efficiency
Date Issued
2022-05
Author(s) USM
DOI
10.1093/mnras/stac1137
Abstract
Common envelope evolution is a fundamental ingredient in our understanding of the formation of close binary stars containing compact objects that include the progenitors of type Ia supernovae, short gamma-ray bursts, and most stellar gravitational wave so
