The double low-mass white dwarf eclipsing binary system J2102-4145 and its possible evolution
In recent years, about 150 low-mass white dwarfs (WDs), typically with masses below 0.4 M ⊙, have been discovered. The majority of these low-mass WDs are observed in binary systems as they cannot be formed through single-star evolution within Hubble time. In this work, we present a comprehensive analysis of the double low-mass WD eclipsing binary
Antunes Amaral, L. et al.
Fecha de publicación:
5
2024