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First release of Master branch

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@rieutord rieutord released this 30 Sep 16:08
· 67 commits to master since this release
r24.10.1-master
2a5da65

This release of the master branch is the first one and is consistent with the description given in papers

  • Espinosa Lara F. and Rieutord M. (2013), ``Self-consistent 2D-models of fast rotating early-type stars", in Astron. Astrophys., vol. 552, A35
  • Rieutord M., Espinosa Lara F. and Putigny B. (2016), ``An algorithm for computing the 2D structure of fast rotating stars", in J. Computational Phys.., vol. 318, 277-304

This version computes the steady state of a two-dimensional model at any rotation rate on the main sequence for masses typically above 1.8 solar mass. The chemical composition is that of GN93 scaled by Z. Details are given in the manual ester.pdf.

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