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Professor De Marco's project and orbital decay

10 AU model will see separating binary stars and others will have orbital decay. 3 AU model will shrink 10% of the separation in 4000 yrs.

Thomas, Professor De Marco's student, communicated with me before. Jonathan and I took a look at their data this morning and find that the effective resolution is 32000. The size of the simulation box is (128000 R_{sun})^{3} and the finest cell is (2.9 R_{sun})^{3}. It need at least 6 levels of AMR.

This job is very computationally intense.

Posted: 8 years ago (Updated: 8 years ago)
Author: Zhuo Chen
Categories: (none)

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orbitaldecay.png (210.0 KB) - added by Zhuo Chen 8 years ago.
3ausidedensity.png (307.2 KB) - added by Zhuo Chen 8 years ago.
3autopdensity.png (141.4 KB) - added by Zhuo Chen 8 years ago.

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