BDSB 93
(MWSC 1030)
0.21
UTI
0.68
CN
1.0
Cdens
0.62
CC3
0.75
Clit
0.28
Cdup
Stellar density (N50/rad)
16.5 [N/pc2]
- CN 0.68 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.62 Intermediate quality
- Clit 0.75 Well-studied
- Cdup 0.28 Possibly duplicate
Overview
BDSB 93 is a moderately populated, very dense object of intermediate C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, very young cluster, but with a large variance across recent sources for the absorption, age, and metallicity parameters (see Parameters). It is well-studied in the literature.
â ī¸ Warning: This is possibly a duplicate object, which shares a significant percentage of members with at least one previously reported entry. See table with shared members information.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 104.304 | -8.221 | 0.748 | -2.447 | 1.119 | 23.384 |
| Almeida et al. | 2025 | 104.295 | -8.215 | â | â | â | â |
| Hunt & Reffert | 2024 | 104.295 | -8.195 | 0.722 | -2.332 | 1.248 | 20.909 |
| Celli et al. | 2024 | 104.297 | -8.202 | â | â | â | â |
| Cavallo et al. | 2024 | 104.418 | -8.384 | 0.726 | â | â | â |
| Hunt & Reffert | 2023 | 104.295 | -8.195 | 0.722 | -2.332 | 1.248 | 20.909 |
| Just et al. | 2023 | 104.288 | -8.188 | â | â | â | â |
| He et al. | 2022 | 104.323 | -8.285 | 0.801 | -1.991 | 0.992 | â |
| Dias et al. | 2021 | 104.295 | -8.215 | 0.751 | -2.389 | 1.021 | â |
| Cantat-Gaudin et al. | 2020 | 104.297 | -8.202 | 0.77 | -2.41 | 1.021 | â |
| Cantat-Gaudin & Anders | 2020 | 104.297 | -8.202 | 0.77 | -2.41 | 1.021 | â |
| Cantat-Gaudin et al. | 2018 | 104.297 | -8.202 | 0.77 | -2.41 | 1.021 | â |
| Kharchenko et al. | 2016 | 104.288 | -8.188 | â | â | â | â |
| Kharchenko et al. | 2013 | 104.295 | -8.19 | â | 3.26 | 0.21 | 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 | 1.25 | 1.915 | 2.24 | 10 | 0.210 | 118 | â | â |
| Almeida et al. | 2025 | 1.02 | 2.23 | â | 12 | â | 153 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 84(1) | â | â |
| Celli et al. | 2024 | â | â | â | 16 | â | 62 | â | â |
| Cavallo et al. | 2024 | 1.25 | 0.74 | â | 81 | 0.530 | â | â | â |
| Hunt & Reffert | 2023 | 1.28 | 1.22 | 2.24 | 7 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 3 | â | 208 | â | â |
| He et al. | 2022 | â | 0.05 | â | 5 | â | â | â | â |
| Dias et al. | 2021 | 1.02 | 2.23 | â | 12 | -0.109 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 1.20 | 1.77 | â | 16 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 1.25 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 1.25 | â | â | â | â | â | â | â |
| Kharchenko et al. | 2016 | 2.17 | 2.06 | â | 3 | â | â | â | â |
| Kharchenko et al. | 2013 | 2.17 | 2.06 | â | 3 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Almeida et al. (2025)
Mass determination: invalid due to poor quality CMD. Isochrone match: worst fit.
Cavallo et al. (2024)
Wood sample.