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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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