Table 3: Here we show the values of χ for main sequence stars derived in the framework of the radial velocity method.
Radial velocity method: c for MSS |
||
Class |
T = 300 K |
T = 4000 K |
O |
~ (1 - 2) × 10-4 |
~ (7.5 - 15) × 10-6 |
B |
~ (0.49 - 1) × 10-4 |
~ (3.6 - 7.5) × 10-6 |
A |
~ (0.42 - 0.49) × 10-4 |
~ (3.2 - 3.6) × 10-6 |
F |
~ (0.38 - 0.42) × 10-4 |
~ (2.8 - 3.2) × 10-6 |
G |
~ (0.34 - 0.38) × 10-4 |
~ (2.6 - 2.8) × 10-6 |
K |
~ (0.28 - 0.34) × 10-4 |
~ (2.1 - 2.6) × 10-6 |
M |
~ (0.16 - 0.28) × 10-4 |
~ (1.2 - 2.1) × 10-6 |