DBSB 157
(MWSC 2367)
0.64
UTI
0.61
CN
0.82
Cdens
1.0
CC3
0.38
Clit
1.0
Cdup
Radius (P>50% members)
4.6 [arcmin]
- CN 0.61 Moderately populated
- Cdens 0.82 Dense
- CC3 1.0 Very high quality
- Clit 0.38 Poorly studied
- Cdup 1.0 Unique
Overview
DBSB 157 is a moderately populated, dense object of very high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a massive, near-solar metallicity, young cluster (see Parameters). It is poorly studied in the literature.
Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.
Distant
Moderate extinction
Massive
Near-solar metallicity
Young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 243.062 | -51.694 | 0.319 | -1.875 | -2.374 | -15.427 |
| Hunt & Reffert | 2024 | 243.076 | -51.721 | 0.332 | -1.864 | -2.401 | -15.292 |
| Cavallo et al. | 2024 | 243.082 | -51.639 | 0.332 | â | â | â |
| Hunt & Reffert | 2023 | 243.076 | -51.721 | 0.332 | -1.864 | -2.401 | -15.292 |
| Just et al. | 2023 | 243.072 | -51.771 | â | â | â | â |
| Kharchenko et al. | 2016 | 243.072 | -51.771 | â | â | â | â |
| Kharchenko et al. | 2013 | 243.084 | -51.771 | â | -4.71 | -3.3 | -67.3 |
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 |
|---|---|---|---|---|---|---|---|---|---|
| Hunt & Reffert | 2024 | â | â | â | â | â | 1333* | â | â |
| Cavallo et al. | 2024 | 2.55 | 2.30 | â | 62 | 0.400 | â | â | â |
| Hunt & Reffert | 2023 | 2.66 | 2.46 | 1.89 | 31 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 89 | â | 3606 | â | â |
| Kharchenko et al. | 2016 | 3.92 | 3.23 | â | 89 | â | â | â | â |
| Kharchenko et al. | 2013 | 3.92 | 3.23 | â | 89 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Gold sample.