BDSB 125
(MWSC 2990)
0.19
UTI
0.53
CN
0.14
Cdens
0.38
CC3
0.0
Clit
0.89
Cdup
Radius (P>50% members)
7.5 [arcmin]
- CN 0.53 Moderately populated
- Cdens 0.14 Very loose
- CC3 0.38 Low quality
- Clit 0.0 Rarely studied
- Cdup 0.89 Very likely unique
Overview
BDSB 125 is a moderately populated, very loose object of low C3 quality. Its parallax locates it at a moderate* distance, near the mid-plane, affected by very high extinction. It is catalogued as a very massive, very young cluster (see Parameters). It is rarely studied in the literature.
(*): The parallax distance estimate (~4.10 kpc) differs significantly from the median photometric distance (~6.70 kpc).
Note: This is very likely a unique object, which shares a 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=0.89) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.
Very distant
Very high extinction
Very massive
Very young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 281.465 | -2.729 | 0.244 | -1.172 | -3.72 | 28.108 |
| Just et al. | 2023 | 281.51 | -2.657 | â | â | â | â |
| Kharchenko et al. | 2016 | 281.51 | -2.657 | â | â | â | â |
| Kharchenko et al. | 2013 | 281.517 | -2.655 | â | 1.29 | -8.99 | 83.3 |
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] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| Just et al. | 2023 | â | â | â | 1 | â | 7780 | â | â |
| Kharchenko et al. | 2016 | 6.70 | 6.45 | â | 1 | â | â | â | â |
| Kharchenko et al. | 2013 | 6.70 | 6.45 | â | 1 | â | â | â | â |
