ASPCS
 
Back to Volume
Paper: Binary Post-AGB Stars
Volume: 313, Asymmetrical Planetary Nebulae III
Page: 536
Authors: van Winckel, H.; Maas, T.; Lloyd-Evans, T.
Abstract: We report here on our ongoing systematic radial velocity monitoring programme of a sample of post-AGB stars. The programme stars are evolved objects with SED characteristics indicative of a dusty disc. The sample was originally tuned to discover new RV Tauri stars (G-K supergiants showing stellar pulsations with alternating deep and shallow minima) by Lloyd Evans (1999). We confirm the suspected high binary fraction.
Back to Volume