arXiv · astro-ph/0702245
Post-AGB Binaries
Abstract
The specific characteristic of the SED of serendipitously discovered post-AGB binaries, allowed us to launch a very extensive multi-wavelength study of evolved objects, selected on the basis of very specific selection criteria. Those criteria were tuned to discover more stars with circumstellar dusty discs. The observational study includes radial velocity monitoring, high spectral resolution optical studies, infrared spectral dust studies, sub-mm bolometric observations and high spatial resolution interferometric experiments with the VLTI. In this contribution, we will review the preliminary results of this program showing that the binary rate is indeed very high. We argue that the formation of a stable circumbinary disc must play a lead role in the evolution of the systems.
Explore related subjects
Keep this discovery
Explore connections, maps & timelines
Hans Van Winckel. 2007-02-09. Post-AGB Binaries. https://arxiv.org/abs/astro-ph/0702245
Cite the original work for its findings. Save a collection to share your selection of sources.