The evolutionary sequences are provided for different stellar masses in the following directories;
| Evolutionary sequences for Grid B |
These are the files
- hr_prems.dat - pre-main sequence evolution
- hr_ms.dat - main sequence evolution
- hr_postms.dat - post-main sequence evolution
| Column | Data | Description |
| 1 | M/Msun | Stellar mass |
| 2 | log(L/Lsun) | Stellar luminosity |
| 3 | Log(Teff) | Effective temperature |
| 4 | R/Rsun | Stellar radius |
| 5 | t | Age in Myrs |
| 6 | Xc | Central Hydrogen abundance |
| 7 | log(g) | Surface gravity in CGS |
| 8 | Nbd | Number of convective borders/transitions |
| 9 | Type | Type of the transitions counting from the centre (and ordered as first-...-last for units-tenths-hundreds-thousands): "1" - from RAD to CONV (start of CZ) "2" - from CONV to RAD (end of CZ) |
| 10 -- 10+Nbd | r_c/R | Location in radius of each transition |
An IDL procedure is also available for producing the HR Diagram with the grid provided. The Plots produced with this procedure are given below.
The mass (in units of solar mass) is indicated by the number near each evolutionary track.
For downloading specific models and/or frequencies please go to the other pages.