Kurucz Models for different stellar types

***This application assumes Solar metalicity

***Stellar Radii are taken from "The Observation and Analysis of Stellar Photospheres", David F. Gray, (Cambridge: Cambridge), 2nd ed., 1992

Type T_{eff} log_g Kurucz model
O5V 44500 4.04 kp00_45000[g50]
O6V 41000 +3.99 kp00_40000[g45]
O8V 35800 +3.94 kp00_35000[g40]
B0V 30000 +3.94 kp00_30000[g40]
B3V 18700 +3.94 kp00_19000[g40]
B5V 15400 +4.04 kp00_15000[g40]
B8V 11900 +4.04 kp00_12000[g40]
A0V 9520 +4.14 kp00_9500[g40]
A5V 8200 +4.29 kp00_8250[g45]
F0V 7200 +4.34 kp00_7250[g45]
F5V 6440 +4.34 kp00_6500[g45]
G0V 6030 +4.39 kp00_6000[g45]
G5V 5770 +4.49 kp00_5750[g45]
K0V 5250 +4.49 kp00_5250[g45]
K5V 4350 +4.54 kp00_4250[g45]
M0V 3850 +4.59 kp00_3750[g45]
M2V 3580 +4.64 kp00_3500[g45]
M5V 3240 +4.94 kp00_3500[g50]
B0III 29000 +3.34 kp00_29000[g35]
B5III 15000 +3.49 kp00_15000[g35]
G0III 5850 +2.94 kp00_5750[g30]
G5III 5150 +2.54 kp00_5250[g25]
K0III 4750 +2.14 kp00_4750[g20]
K5III 3950 +1.74 kp00_4000[g15]
M0III 3800 +1.34 kp00_3750[g15]
O5I 40300 +3.34 kp00_40000[g45]
O6I 39000 +3.24 kp00_40000[g45]
O8I 34200 +3.24 kp00_34000[g40]
BOI 26000 +2.84 kp00_26000[g30]
B5I 13600 +2.44 kp00_14000[g25]
AOI 9730 +2.14 kp00_9750[g20]
A5I 8510 +2.04 kp00_8500[g20]
F0I 7700 +1.74 kp00_7750[g20]
F5I 6900 +1.44 kp00_7000[g15]
G0I 5550 +1.34 kp00_5500[g15]
G5I 4850 +1.14 kp00_4750[g10]
K0I 4420 +0.94 kp00_4500[g10]
K5I 3850 +0.34 kp00_3750[g05]
M0I 3650 +0.14 kp00_3750[g00]
M2I 3450 -0.06 kp00_3500[g00]