Table 5:
Theoretical colours of M- and C-stars of solar metallicity.
For some models, the second line indicates the colours when the star is
obscured by circumstellar dust equivalent to a dimming in K by 0.05 mag.
| SpT |
 |
(I-J) |
(J-K) |
| M 0 |
3850 |
1.18 |
1.08 |
| M 3 |
3550 |
1.39 |
1.18 |
| M 3 + dust |
3550 |
1.53 |
1.34 |
| M 5 |
3397 |
1.86 |
1.27 |
| M 7 |
3129 |
3.11 |
1.37 |
| M 7 + dust |
3129 |
3.73 |
1.97 |
| M 8 |
2890 |
3.71 |
1.37 |
| M 10 |
2500 |
4.13 |
1.35 |
| M 10 + dust |
2500 |
4.45 |
1.74 |
| C |
3600 |
1.43 |
1.17 |
| C |
3400 |
1.56 |
1.30 |
| C |
3200 |
1.72 |
1.43 |
| C |
2800 |
2.00 |
1.61 |
| C |
2650 |
2.09 |
1.61 |
| C + dust |
2650 |
2.48 |
2.09 |
Source LaTeX |
All tables |
In the text