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| Paper: |
Orbiting Dust Disks Around Evolved Stars |
| Volume: |
313, Asymmetrical Planetary Nebulae III |
| Page: |
493 |
| Authors: |
Jura, M. |
| Abstract: |
There is now strong evidence that some post main sequence stars have substantial amounts of gravitationally bound, orbiting, circumstellar dust. The best studied case is HD 44179, the Red Rectangle, where the orbiting circumstellar disk possesses a significant fraction of the total angular momentum of the system. |
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