BDSB 91
(MWSC 861)
0.78
UTI
0.6
CN
1.0
Cdens
0.75
CC3
0.78
Clit
1.0
Cdup
Stellar density (N50/rad)
59.7 [N/pc2]
- CN 0.6 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.78 Well-studied
- Cdup 1.0 Unique
Overview
BDSB 91 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a close distance, below 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 age parameter (see Parameters). It is well-studied in the literature.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 96.318 | -10.558 | 1.094 | -3.169 | 1.29 | 27.772 |
| Almeida et al. | 2025 | 96.329 | -10.546 | â | â | â | â |
| Alfonso et al. | 2024 | 97.701 | -9.55 | 0.981 | -3.202 | 0.652 | â |
| Hunt & Reffert | 2024 | 96.316 | -10.558 | 1.049 | -3.125 | 1.229 | 41.44 |
| Celli et al. | 2024 | 96.319 | -10.551 | â | â | â | â |
| Cavallo et al. | 2024 | 96.34 | -10.536 | 1.09 | â | â | â |
| Hunt & Reffert | 2023 | 96.316 | -10.558 | 1.049 | -3.125 | 1.229 | 41.44 |
| Just et al. | 2023 | 96.316 | -10.553 | â | â | â | â |
| He et al. | 2022 | 96.322 | -10.55 | 1.105 | -3.143 | 1.237 | â |
| Dias et al. | 2021 | 96.329 | -10.546 | 1.018 | -3.101 | 1.164 | â |
| Cantat-Gaudin et al. | 2020 | 96.319 | -10.551 | 1.033 | -3.183 | 1.15 | â |
| Cantat-Gaudin & Anders | 2020 | 96.319 | -10.551 | 1.033 | -3.183 | 1.15 | â |
| Cantat-Gaudin et al. | 2018 | 96.319 | -10.551 | 1.033 | -3.183 | 1.15 | â |
| Kharchenko et al. | 2016 | 96.316 | -10.553 | â | â | â | â |
| Kharchenko et al. | 2013 | 96.322 | -10.555 | â | 0.21 | -0.74 | 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 | 0.95 | 1.55 | 2.2 | 5 | 0.007 | 123 | â | â |
| Almeida et al. | 2025 | 0.91 | 1.47 | â | 5 | â | 110 | â | â |
| Alfonso et al. | 2024 | 0.96 | 1.80 | â | 44 | 0.007 | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 83(1) | â | â |
| Celli et al. | 2024 | â | â | â | 14 | â | 136 | â | â |
| Cavallo et al. | 2024 | 1.45 | 1.46 | â | 91 | 0.090 | â | â | â |
| Hunt & Reffert | 2023 | 0.86 | 1.55 | 2.20 | 5 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 4 | â | 176 | â | â |
| He et al. | 2022 | â | 1.55 | â | 5 | â | â | â | â |
| Dias et al. | 2021 | 0.91 | 1.47 | â | 5 | 0.007 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.96 | 1.80 | â | 14 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.94 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 0.94 | â | â | â | â | â | â | â |
| Kharchenko et al. | 2016 | 1.92 | 4.19 | â | 4 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.92 | 4.19 | â | 4 | 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: intermediate fit. Isochrone match: good fit.
Cavallo et al. (2024)
Wood sample.