Formation of long-period post-common-envelope binaries I. No extra energy is needed to explain oxygen-neon white dwarfs paired with AFGK-type main-sequence stars

Ähnliche Einträge

• Formation of long-period post-common-envelope binaries II. Explaining the self-lensing binary KOI 3278
  von: Belloni, Diogo, et al.
  Veröffentlicht: (2024)
• Reconstructing post-common envelope white dwarf+main sequence binary histories through inverse population synthesis techniques
  von: Torres, Santiago, et al.
  Veröffentlicht: (2025)
• The incidence of magnetic cataclysmic variables can be explained by the late appearance of white dwarf magnetic fields
  von: Schreiber, Matthias R., et al.
  Veröffentlicht: (2025)
• An eclipsing CEMP candidate discovered in a search for dwarf carbon stars in post-common envelope binaries
  von: McLennan, Jonathan A. G., et al.
  Veröffentlicht: (2026)
• The white dwarf binary pathways survey -- X. Gaia orbits for known UV excess binaries
  von: Garbutt, J. A., et al.
  Veröffentlicht: (2024)