Table 10:
Effective temperature scales of B-type stars in the Milky Way, LMC and SMC for
different luminosity classes. These scales are based on parameters presented in this
paper and Paper IV, as well as a number of SMC stars from Dufton et al. (2005). The
values in parenthesis are those for which we have no objects in the spectral type bin
but for which we could interpolate. The
values are presented in units of K.
|
Milky Way |
LMC |
SMC |
Sp. Typ. |
V |
I |
III |
V |
I |
III |
V |
B0 |
30 650 |
28 550 |
29 100 |
31 400 |
27 200 |
|
32 000 |
B0.2 |
[29 050] |
[26 950] |
[27 850] |
30 250 |
[25 750] |
|
30 800 |
B0.5 |
27 500 |
25 350 |
[26 650] |
29 100 |
[24 300] |
|
29 650 |
B0.7 |
[25 900] |
23 750 |
[25 400] |
[27 950] |
[22 850] |
25 300 |
28 450 |
B1 |
24 300 |
22 150 |
24 150 |
26 800 |
22 350 |
23 950 |
27 300 |
B1.5 |
22 700 |
20 550 |
22 950 |
25 700 |
20 650 |
[22 550] |
[26 100] |
B2 |
22 100 |
18 950 |
21 700 |
24 550 |
18 950 |
21 200 |
24 950 |
B2.5 |
19 550 |
17 350 |
20 450 |
23 400 |
17 200 |
19 850 |
|
B3 |
17 950 |
15 750 |
19 250 |
|
15 500 |
18 450 |
|
B5 |
|
14 150 |
|
|
13 800 |
|
|
B8 |
|
12 550 |
|
|
|
|
|
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