DBSB 165
(DBSB2003 165; DBS2003 165)
0.05
UTI
0.0
CN
0.04
Cdens
0.25
CC3
0.0
Clit
0.96
Cdup
Nm (P>50%)
19
Core radius and density
5.3 [pc], 0.2 [pc-2]
- CN 0.0 Sparse
- Cdens 0.04 Very loose
- CC3 0.25 Low quality
- Clit 0.0 Rarely studied
- Cdup 0.96 Unique
Overview
DBSB 165 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate distance, near the mid-plane. It is catalogued as a very young cluster (see Parameters). It is rarely studied in the literature, with no articles listed in the last 13 years.
Note: This is a unique object, which shares a very small percentage of members with at least one previously reported entry. See table with shared members information.
â ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=0.96) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 245.429 | -50.422 | 0.401 | -2.767 | -4.112 | -33.855 |
| Morales et al. | 2013 | 245.379 | -50.418 | â | â | â | â |
| Dutra et al. | 2003 | 245.377 | -50.412 | â | â | â | â |
đĄ Note: The UCC values are estimated from its identified members.
| Reference | Year | Dist [kpc] | Av [mag] | DAv [mag] | Age [Myr] | [Fe/H] [dex] | Mass [Msun] | Bfrac | BSS |
|---|---|---|---|---|---|---|---|---|---|
| UCC | 99999â | 3.49 | â | â | 3 | â | â | â | â |
| Morales et al. | 2013 | 3.49 | â | â | 3 | â | â | â | â |
MOCA

Morales et al. (2013)
Classified as morphological type 'EC1' (deeply embedded cluster). Morphological flag: cluster fully embedded, presence of emission related to PAH or warm dust.
Dutra et al. (2003)
Classified as infrared cluster (IRC).