The GYRE Forums

Hi Rich, Thanks for all the great work on GYRE! Using the most recent version of GYRE (that came with the MESA distribution) I still find problems with computing the local work in a strongly adiabatic environment (e.g., white dwarf interiors). I know this is a generic problem that all nonadiabatic p...

Hi Rich, First of all, I tried what you suggested. It helps with some of the noise in the deep interior but that's not really what I'm talking about. I think there must be a fundamental problem with the way dW_dx is being calculated, and also (possibly) with the non adiabatic results the code gives ...

Hi Rich, I'm having some trouble with non adiabatic calculations of white dwarf models. Basically, I expect dW_dx to be small everywhere except in the outer layers, but the opposite seems to be the case. I'm attaching plots of example calculations I've done of a 0.15 Msun WD. The bumps that I see at...

Hi Rich, I just tried to do an update of gyre by doing hg pull hg update in each of the 3 gyre directories build, core and gyre. On both of my macs I get the same compile error when compiling, for example, in the ad directory: ix|~/gyre/gyre/ad> make fpx3_deps -DGFORTRAN_PR_56052 -DGFORTRAN_PR_56872...

Hi Rich, > > 1. I know it may be redundant, but could some or all of the Gyre output files contain > > header information about the stellar model that was used, i.e., its Teff, Luminosity, > > Age, Mass, metallicity, etc.? This would be really great. > > > > I can easily put this in the screen outpu...

Hi Rich, Thanks for setting up this website and making Gyre available! Just off the top of my head I have a couple a requests on my wish list. 1. I know it may be redundant, but could some or all of the Gyre output files contain header information about the stellar model that was used, i.e., its Tef...