par Dermine, Tijl ;Jorissen, Alain ;Izzard, Robert ;Church, Ross R.P.
Référence AIP Conference Proceedings, 1314, page (61-62)
Publication Publié, 2010
Article révisé par les pairs
Résumé : The barium overabundances observed at the surface of barium stars originate from accretion long ago from the wind of a companion AGB star. However, this scenario cannot explain their high eccentricities and short orbital periods that have remained a mystery for decades. We investigate how kicks imparted to the white-dwarf at its birth or the presence of a circumbinary disk can solve this problem. © 2010 American Institute of Physics.