Table 7:
Data used for the SED-calculations,
V-magnitude with references for each photometric observation.
Observations on the WULBV (Walraven) photometric system can be found in
deWinter et al. (2001) with the exception of HD 139614 and SU Aur.
Observations in the 4 IRAS bands (11.8, 24.4, 58.6 and 101
m) can be
found in NASA RP-1190 (1988).
PMS star |
UBVRI |
JHKLM |
HD 97048 |
8.461,5,11 |
8.461,5,11 |
UX Ori |
10.9112 |
10.9212 |
HD 163296 |
6.9015, 6.885 |
6.9015, 6.885 |
V380 Ori |
10.4811,10.4410 |
10.4811,10.4411 |
HK Ori |
11.5211,11.6510 |
11.6311,11.6510 |
KK Oph |
11.825 |
11.915 |
BF Ori |
11.045 |
11.035 |
HR 5999 |
6.8110 |
6.8010 |
HD 139614 |
8.2614 |
8.2614 |
V351 Ori |
8.925 |
8.925 |
HD 104237 |
6.609 |
6.609 |
BN Ori |
9.6813 |
9.6813 |
CQ Tau |
9.82,9.457 |
9.457 |
NX Pup |
10.243, 10.643 |
10.143 |
AK Sco |
8.95, 9.03, 8.96, 9.0410 |
8.95, 9.02, 9.0410 |
SU Aur |
9.024, 9.098, 9.1512 |
9.024, 9.078, 9.1512 |
1: |
| vandenAncker (1996) |
9: |
| Hu et al. (1989) |
2: |
| Berdyugin et al. (1990, 1992) |
10: |
| Kilkenny et al. (1985) |
3: |
| Brand et al. (1983) |
11: |
| Remijn (1980) |
4: |
| Cohen & Schwartz (1976) |
12: |
| Rydgren et al. (1976) |
5: |
| deWinter et al. (2001) |
13: |
| Shevchenko et al. (1997) |
7: |
| Eiroa et al. (2002) |
14: |
| Sylvester et al. (1967) |
8: |
| Eugenio & Mendoza (1966) |
15: |
| Thé et al. (1985a) |
Source LaTeX |
All tables |
In the text