Binary Post-AGB Stars

Details Binary Post-AGB Stars Binary Post-AGB Stars

Jul 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aspc..313..536v&link_type=abstract

Asymmetrical Planetary Nebulae III: Winds, Structure and the Thunderbird, Proceedings of the conference held 28 July - 1 August

Astronomy and Astrophysics

Astronomy

Scientific paper

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.

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