Two almost planetary mass survivors of common envelope evolution
White dwarfs are often found in close binaries with stellar or even substellar companions. It is generally thought that these compact binaries form via common envelope evolution, triggered by the progenitor of the white dwarf expanding after it evolved off the main sequence and engulfing its companion. To date, a handful of white dwarfs in compact
Parsons, S. G. et al.
Fecha de publicación:
2
2025