DBSB 175
(DBS2003 175; MWSC 2478)
0.15
UTI
0.0
CN
0.12
Cdens
0.12
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad)
0.6 [N/pc2]
- CN 0.0 Sparse
- Cdens 0.12 Very loose
- CC3 0.12 Very low quality
- Clit 0.25 Poorly studied
- Cdup 1.0 Unique
Overview
DBSB 175 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a moderate* distance, near the mid-plane, affected by high extinction. It is catalogued as a very young cluster (see Parameters). It is poorly studied in the literature.
(*): The parallax distance estimate (~2.42 kpc) differs significantly from the median photometric distance (~3.80 kpc).
Note: This object shares a small percentage of members with 2 later reported entries. See table with shared members information.
â ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) 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 | 253.065 | -43.421 | 0.414 | -1.262 | -3.815 | -23.938 |
| Just et al. | 2023 | 253.137 | -43.396 | â | â | â | â |
| Kharchenko et al. | 2016 | 253.137 | -43.396 | â | â | â | â |
| Kharchenko et al. | 2013 | 253.147 | -43.396 | â | -2.69 | -2.03 | -45.9 |
| Morales et al. | 2013 | 253.15 | -43.391 | 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 | 3.8 | 3.87 | â | 1 | â | 632 | â | â |
| Just et al. | 2023 | â | â | â | 1 | â | 632 | â | â |
| Kharchenko et al. | 2016 | 3.80 | 3.87 | â | 1 | â | â | â | â |
| Kharchenko et al. | 2013 | 3.80 | 3.87 | â | 1 | â | â | â | â |
| Morales et al. | 2013 | 5.01 | â | â | â | â | â | â | â |
MOCA

Morales et al. (2013)
Classified as morphological type 'EC2' (partially embedded cluster). Morphological flag: cluster partially embedded, presence of an IR bubble.