Post common envelope binaries from SDSS. XIII. Mass dependencies of the orbital period distribution
Context. Post-common-envelope binaries (PCEBs) consisting of a white dwarf (WD) and a main-sequence secondary star are ideal systems to constrain models of common-envelope (CE) evolution. Until very recently, observed samples of PCEBs have been too small to fully explore this potential, however the recently identified large and relatively
Zorotovic, M. et al.
Fecha de publicación:
12
2011