The old page of Y2 can be accessed as well.
- You can try out the Y2 version 3 !
Download the isochrone sets of Y2 version 3
When downloaded, ungzipped and untared, an interpolation program together with the isochrones can be found.
This is for interpolation in Y, [a/Fe], Z, and age.
Download the evolution track sets of Y2 version 3
This gzipped tared file contains both of the base set and the wider Y set as well as an interpolation program.
The first announcement of the 3rd version has been; Yi, S. K., Kim, Y. -C., Demarque, P., Lee, Y. W., Han, S.-I. and Kim, D. G. `The Y2 Isochrones getting an extra dimension' (2008) The Art of Modelling Stars in the 21st Century, IAU Symposium 252, held 6-11 April 2008 at Sanya, China, 413 -- 416
The HB tracks (Han, S.-I. et al. 2009) will be on-line soon.
We acknowledge the significant contribution of C. Na, S. -I. Han, and D. G. Kim, to this 3rd version.
The 3rd version Y2 is consisted of 2 sets. The base set is for Y = dY/dZ * Z + Yp where dY/dZ = 1.5, 2.0, 2.5, and 3.0, with Yp=0.23
Thus, the range of Y is narrower in lower Z. The extra set for wider range of Y is for Y = dY/dZ * Z + Yp where Yp = 0.23, 0.28, 0.33, 0.38, and 0.43, with dY/dZ=2.0
The coverage of the base set The coverage of the extra set for wider range of Y Z [a/Fe]=0.0, [a/Fe]=0.3, [a/Fe]=0.6 dY/dZ=1.5 dY/dZ=2.0 dY/dZ=2.5 dY/dZ=3.0 0.00001 O O O O 0.0001 O O O O 0.0004 O O O O 0.001 O O O O 0.004 O O O O 0.007 O O O O 0.01 O O O O 0.02 O O O O 0.04 O O O O 0.06 O O O 0.08 O O O Z [a/Fe]=0.3 Yp=0.23 Yp=0.28 Yp=0.33 Yp=0.38 Yp=0.43 0.00001 O O O O O 0.0001 O O O O O 0.0004 O O O O O 0.001 O O O O O 0.004 O O O O O 0.007 O O O O O 0.01 O O O O O 0.02 O O O O O 0.04 O 0.06 O 0.08 O Y = dY/dZ * Z + Yp, for Yp=0.23 Y = dY/dZ * Z + Yp, for dY/dZ=2.0
Summary of the input physics
Grevesse and Noels Solar mixture OPAL EOS OPAL Rosseland mean Opacities and Ferguson Low temperature opacities Bahcall and Pinsonneault Energy generation rates Itoh et al. Neutrino loss rate Convective core overshoot ~0.2Hp Thoul et al. Helium diffusion Eddington grey Atmosphere
The EEP mapping scheme (Kim, D. G., 2005, MS thesis, Yonsei University)
The 9 Primary EEPs are identified first, and then the secondary EEPs are set in between, in equal spacing.