BDSB 90
(MWSC 1053)
0.21
UTI
0.0
CN
1.0
Cdens
0.38
CC3
0.0
Clit
0.76
Cdup
Stellar density (N50/rad)
9.9 [N/pc2]
- CN 0.0 Sparse
- Cdens 1.0 Very dense
- CC3 0.38 Low quality
- Clit 0.0 Rarely studied
- Cdup 0.76 Very likely unique
Overview
BDSB 90 is a sparse, very dense object of low C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a very young cluster (see Parameters). It is rarely studied in the literature.
Note: This is very likely a unique object, which shares a small percentage of members with at least one previously reported entry, and a very small percentage with at least one entry reported in the same catalogue. See table with shared members information.
â ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=0.76) 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 | 104.887 | -4.812 | 0.438 | -1.488 | 0.611 | 62.256 |
| Just et al. | 2023 | 104.903 | -4.858 | â | â | â | â |
| Kharchenko et al. | 2016 | 104.903 | -4.858 | â | â | â | â |
| Kharchenko et al. | 2013 | 104.91 | -4.86 | â | 0.85 | -0.34 | 41.0 |
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 | 2.66 | 2.65 | â | 16 | â | 150 | â | â |
| Just et al. | 2023 | â | â | â | 16 | â | 150 | â | â |
| Kharchenko et al. | 2016 | 2.66 | 2.65 | â | 16 | â | â | â | â |
| Kharchenko et al. | 2013 | 2.66 | 2.65 | â | 16 | â | â | â | â |
MOCA
