BDSB 104
(BDS2003 104)
0.26
UTI
0.45
CN
0.08
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Nm (P>50%)
45
Core radius and density
2.3 [pc], 0.4 [pc-2]
- CN 0.45 Poorly populated
- Cdens 0.08 Very loose
- CC3 0.75 High quality
- Clit 0.0 Rarely studied
- Cdup 1.0 Unique
Overview
BDSB 104 is a poorly populated, very loose object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane. No fundamental parameter values are available for this object. It is rarely studied in the literature, with no articles listed in the last 13 years.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 268.571 | -25.847 | 0.361 | -0.157 | -1.017 | -63.313 |
| Morales et al. | 2013 | 268.604 | -25.86 | â | â | â | â |
| Bica et al. | 2003 | 268.607 | -25.864 | â | â | â | â |
đĄ Note: The UCC values are estimated from its identified members.
MOCA

Morales et al. (2013)
Classified as morphological type 'OC0' (emerging exposed cluster). Morphological flag: possibly associated submm emission surrounding the cluster.
Bica et al. (2003)
Classified as stellar group (IRGr).