UBC 1303
0.60
UTI
0.62
CN
1.0
Cdens
0.75
CC3
0.31
Clit
1.0
Cdup
Radius (P>50% members)
4.5 [arcmin]
- CN 0.62 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.31 Poorly studied
- Cdup 1.0 Unique
Overview
UBC 1303 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It is poorly studied in the literature.
Note: This object shares a significant percentage of members with 2 later reported entries. See table with shared members information.
Relatively close
Moderate extinction
Near-solar metallicity
Intermediate age
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 92.009 | 21.918 | 0.506 | 0.925 | -3.57 | 11.106 |
| Zhang et al. | 2024 | 91.993 | 21.915 | â | â | â | â |
| Hunt & Reffert | 2024 | 91.993 | 21.915 | 0.504 | 0.89 | -3.511 | 3.915 |
| Cavallo et al. | 2024 | 91.997 | 21.926 | 0.505 | â | â | â |
| Hunt & Reffert | 2023 | 91.993 | 21.915 | 0.504 | 0.89 | -3.511 | 3.915 |
| Castro-Ginard et al. | 2022 | 91.98 | 21.93 | 0.51 | 0.94 | -3.6 | 11.38 |
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 |
|---|---|---|---|---|---|---|---|---|---|
| Zhang et al. | 2024 | â | â | â | â | -0.138* | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 307* | â | â |
| Cavallo et al. | 2024 | 1.91 | 1.30 | â | 331 | 0.540 | â | â | â |
| Hunt & Reffert | 2023 | 1.81 | 1.28 | 1.19 | 244 | â | â | â | â |
| Castro-Ginard et al. | 2022 | 2.02 | 1.00 | â | 301 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Gold sample.