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Paper: Post-AGB Binaries and Their Connection to the B[e] Phenomenon
Volume: 508, The B[e] Phenomenom: Forty Years of Studies
Page: 197
Authors: Van Winckel, H.
Abstract: We argue in this contribution that secondary stable disks around evolved stars can be found over a wide range in luminosity all over the HR-diagram. The disks around B[e] supergiants form the high luminosity end of similar structures found around post-Asymptotic Giant Branch (post-AGB) stars as well as the recently discovered post-Red Giant Branch (post-RGB) stars. We focus here on the observational properties of disks around binary post-AGB stars and end with a link to the B[e] phenomenon.
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