Name | d (pc) | Tk (K) | ![]() |
![]() |
M (![]() |
D (pc) |
![]() ![]() |
Total | 1.55 ![]() |
19.0 ![]() |
1.54 ![]() |
1.73 ![]() |
1500 ![]() |
3580 ![]() |
25900 ![]() |
Group I | 1.61 ![]() |
19.7 ![]() |
1.65 ![]() |
1.75 ![]() |
1800 ![]() |
4000 ![]() |
29000 ![]() |
Group II | 1.66 ![]() |
17.7 ![]() |
1.50 ![]() |
1.67 ![]() |
940 ![]() |
3200 ![]() |
(24000 ![]() |
Cepheus (far)1 | 0.96 ![]() |
20.4 ![]() |
1.5 ![]() |
590 ![]() |
3500 | 25000 ![]() |
|
Taurus2 | 0.10 ![]() |
10.0 ![]() |
0.30 ![]() |
9 ![]() |
140 | 1.1 ![]() |
Note:
1. Harju et al. (1993);
2. Benson & Myers (1989), data taken from ref. 1
directly;
3. The value in parentheses is the luminosity
of the IRAS sources for the group II. |