![]() |
![]() |
Figure 5:
The T(K) = 3500, [![]() |
![]() |
Figure 6:
The T(K) = 3500, [![]() |
![]() |
Figure 7:
The T(K) = 3500, [![]() |
![]() |
Figure 8:
The T(K) = 3500, [![]() |
![]() |
Figure 9:
The T(K) = 3500, [Z/Z![]() |
![]() |
Figure 10:
The T(K) = 3750, [![]() |
![]() |
Figure 11:
The T(K) = 3750, [![]() |
![]() |
Figure 12:
The T(K) = 3750, [![]() |
![]() |
Figure 13:
The T(K) = 3750, [![]() |
![]() |
Figure 14:
The T(K) = 3750, [![]() |
![]() |
Figure 15:
The T(K) = 4000, [![]() |
![]() |
Figure 16:
The T(K) = 4000, [![]() |
![]() |
Figure 17:
The T(K) = 4000, [![]() |
![]() |
Figure 18:
The T(K) = 4000, [![]() |
![]() |
Figure 19:
The T(K) = 4000, [![]() |
![]() |
Figure 20:
The T(K) = 4250, [![]() |
![]() |
Figure 21:
The T(K) = 4250, [![]() |
![]() |
Figure 22:
The T(K) = 4250, [![]() |
![]() |
Figure 23:
The T(K) = 4250, [![]() |
![]() |
Figure 24:
The T(K) = 4250, [![]() |
![]() |
Figure 25:
The T(K) = 4500, [![]() |
![]() |
Figure 26:
The T(K) = 4500, [![]() |
![]() |
Figure 27:
The T(K) = 4500, [![]() |
![]() |
Figure 28:
The T(K) = 4500, [![]() |
![]() |
Figure 29:
The T(K) = 4500, [![]() |
![]() |
Figure 30:
The T(K)=4750, [![]() |
![]() |
Figure 31:
The T(K) = 4750, [![]() |
![]() |
Figure 32:
The T(K) = 4750, [![]() |
![]() |
Figure 33:
The T(K) = 4750, [![]() |
![]() |
Figure 34:
The T(K) = 4750, [![]() |
![]() |
Figure 35:
The T(K) = 5000, [![]() |
![]() |
Figure 36:
The T(K) = 5000, [![]() |
![]() |
Figure 37:
The T(K) = 5000, [![]() |
![]() |
Figure 38:
The T(K) = 5000, [![]() |
![]() |
Figure 39:
The T(K) = 5000, [![]() |
![]() |
Figure 40:
The T(K) = 5250, [![]() |
![]() |
Figure 41:
The T(K) = 5250, [![]() |
![]() |
Figure 42:
The T(K) = 5250, [![]() |
![]() |
Figure 43:
The T(K) = 5250, [![]() |
![]() |
Figure 44:
The T(K) = 5250, [![]() |
![]() |
Figure 45:
The T(K) = 5500, [![]() |
![]() |
Figure 46:
The T(K) = 5500, [![]() |
![]() |
Figure 47:
The T(K) = 5500, [![]() |
![]() |
Figure 48:
The T(K) = 5500, [![]() |
![]() |
Figure 49:
The T(K) = 5500, [![]() |
![]() |
Figure 50:
The T(K) = 5750, [![]() |
![]() |
Figure 51:
The T(K) = 5750, [![]() |
![]() |
Figure 52:
The T(K) = 5750, [![]() |
![]() |
Figure 53:
The T(K) = 5750, [![]() |
![]() |
Figure 54:
The T(K) = 5750, [![]() |
![]() |
Figure 55:
The T(K) = 6000, [![]() |
![]() |
Figure 56:
The T(K) = 6000, [![]() |
![]() |
Figure 57:
The T(K) = 6000, [![]() |
![]() |
Figure 58:
The T(K) = 6000, [![]() |
![]() |
Figure 59:
The T(K) = 6000, [![]() |
![]() |
Figure 60:
The T(K) = 6250, [![]() |
![]() |
Figure 61:
The T(K) = 6250, [![]() |
![]() |
Figure 62:
The T(K) = 6250, [![]() |
![]() |
Figure 63:
The T(K) = 6250, [![]() |
![]() |
Figure 64:
The T(K) = 6250, [![]() |
![]() |
Figure 65:
The T(K) = 6500, [![]() |
![]() |
Figure 66:
The T(K) = 6500, [![]() |
![]() |
Figure 67:
The T(K) = 6500, [![]() |
![]() |
Figure 68:
The T(K) = 6500, [![]() |
![]() |
Figure 69:
The T(K) = 6500, [![]() |
![]() |
Figure 70:
The T(K) = 6750, [![]() |
![]() |
Figure 71:
The T(K) = 6750, [![]() |
![]() |
Figure 72:
The T(K) = 6750, [![]() |
![]() |
Figure 73:
The T(K) = 6750, [![]() |
![]() |
Figure 74:
The T(K) = 6750, [![]() |
![]() |
Figure 75:
The T(K) = 7000, [![]() |
![]() |
Figure 76:
The T(K) = 7000, [![]() |
![]() |
Figure 77:
The T(K) = 7000, [![]() |
![]() |
Figure 78:
The T(K) = 7000, [![]() |
![]() |
Figure 79:
The T(K) = 7000, [![]() |
![]() |
Figure 80:
The T(K) = 7250, [![]() |
![]() |
Figure 81:
The T(K) = 7250, [![]() |
![]() |
Figure 82:
The T(K) = 7250, [![]() |
![]() |
Figure 83:
The T(K) = 7250, [![]() |
![]() |
Figure 84:
The T(K) = 7250, [![]() |
![]() |
Figure 85:
The T(K) = 7500, [![]() |
![]() |
Figure 86:
The T(K) = 7500, [![]() |
![]() |
Figure 87:
The T(K)=7500, [![]() |
![]() |
Figure 88:
The T(K) = 7500, [![]() |
![]() |
Figure 89:
The T(K) = 7500, [![]() |
![]() |
Figure 90:
The observed solar spectrum from Kurucz et al. (1984) ATLAS
(degraded to a resolving power ![]() ![]() |
![]() |
Figure 91: The spectrum of the G5 V star HD 20630 from Paper I compared to the closest synthetic spectrum from the grid computed in this paper |
![]() |
Figure 92: The spectrum of the K5 V star HD 201091 from Paper I compared to the closest synthetic spectrum from the grid computed in this paper |
Copyright The European Southern Observatory (ESO)