Post-common envelope binaries from SDSS - XVI. Long orbital period systems and the energy budget of common envelope evolution
Virtually all close compact binary stars are formed through common envelope (CE) evolution. It is generally accepted that during this crucial evolutionary phase a fraction of the orbital energy is used to expel the envelope. However, it is unclear whether additional sources of energy, such as the recombination energy of the envelope, play an
Rebassa-Mansergas, A. et al.
Fecha de publicación:
6
2012