Table 1.
Relevant characteristics of our sequences a Teff = 10 000 K.
| MWD | MG | RNewt | RGR | log gNewt | log gGR |  |
 |
|---|---|---|---|---|---|---|---|
| (M⊙) | (M⊙) | (km) | (km) | (cm s−2) | (cm s−2) | (g cm−3) | (g cm−3) |
| 1.29 | 1.28977 | 2685.40 | 2608.86 | 9.375 | 9.401 | 6.71 × 108 | 7.51 × 108 |
| 1.31 | 1.30976 | 2426.04 | 2326.17 | 9.470 | 9.507 | 9.98 × 108 | 1.17 × 109 |
| 1.33 | 1.32974 | 2156.90 | 2004.60 | 9.579 | 9.643 | 1.57 × 109 | 2.06 × 109 |
| 1.35 | 1.34972 | 1829.29 | 1542.51 | 9.728 | 9.878 | 2.90 × 109 | 5.36 × 109 |
| 1.369 | 1.36871 | 1408.77 | 1051.16 | 9.961 | 10.217 | 7.42 × 109 | 2.11 × 1010 |
Notes. MWD: total baryonic mass. MG: total gravitational mass. RNewt: stellar radius in the Newtonian case. RGR: stellar radius in the general relativity case. gNewt: surface gravity in the Newtonian case. gGR: surface gravity in the general relativity case. 
: central density of rest mass in the Newtonian case. 
: central density of rest mass in the general relativity case.
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