Class bamr::bamr_class

Right now the EOS is rejected if the pressure decreases at any density, when in reality, it should only check if the pressure decreases at a density below that of the central density of the maximum mass star. This isn't a problem for current EOSs, but could be a problem in the future.

It's not clear if successive calls of the mcmc command really work. For now, one may have ensure the program exits after each mcmc() run.

Fix issue of block_counter giving confusing output if there are too few MCMC points between each block.

More testing

Better documentation

Help with plots

Global bamr::bamr_class::compute_star (entry &e, model &modref, o2scl::tov_solve *ts, int &success)

Temporarily made public for drdp project hack