UBC 1272
0.55
UTI
0.36
CN
1.0
Cdens
0.75
CC3
0.31
Clit
1.0
Cdup
Radius (P>50% members)
4.2 [arcmin]
- CN 0.36 Poorly populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.31 Poorly studied
- Cdup 1.0 Unique
Overview
UBC 1272 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, below 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 large percentage of members with a later reported entry. 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 | 68.698 | 38.395 | 0.599 | 0.592 | -3.228 | -15.713 |
| Zhang et al. | 2024 | 68.72 | 38.393 | â | â | â | â |
| Hunt & Reffert | 2024 | 68.72 | 38.393 | 0.591 | 0.577 | -3.25 | 0.503 |
| Cavallo et al. | 2024 | 68.692 | 38.406 | 0.592 | â | â | â |
| Hunt & Reffert | 2023 | 68.72 | 38.393 | 0.591 | 0.577 | -3.25 | 0.503 |
| Castro-Ginard et al. | 2022 | 68.71 | 38.39 | 0.59 | 0.58 | -3.25 | 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] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| Zhang et al. | 2024 | â | â | â | â | -0.072* | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 252* | â | â |
| Cavallo et al. | 2024 | 1.28 | 2.19 | â | 427 | -0.790 | â | â | â |
| Hunt & Reffert | 2023 | 1.65 | 1.90 | 2.21 | 259 | â | â | â | â |
| Castro-Ginard et al. | 2022 | 1.81 | 1.33 | â | 75 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Gold sample.