Nebot Gomez-Moran A.; Gansicke B.T.; Schreiber M.R.; Rebassa-Mansergas A.; Schwope A.D.; Southworth J.; Aungwerojwit A.; Bothe M.; Davis P.J.; Kolb U.; Muller M.; Papadaki C.; Pyrzas S.; Rabitz A.; Rodriguez-Gil P.; Schmidtobreick L.; Schwarz R.; Tappert C.; Toloza O.; Vogel J.; Zorotovic M.
(2014-04-04)
Context. The complexity of the common-envelope phase and of magnetic stellar wind braking currently limits our understanding of close binary evolution. Because of their intrinsically simple structure, observational population ...