Ruprecht 123
(MWSC 2584)
0.37
UTI
0.0
CN
0.09
Cdens
0.12
CC3
0.82
Clit
1.0
Cdup
Radius (P>50% members)
11.0 [arcmin]
- CN 0.0 Sparse
- Cdens 0.09 Very loose
- CC3 0.12 Very low quality
- Clit 0.82 Well-studied
- Cdup 1.0 Unique
Overview
Ruprecht 123 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a relatively close distance, near 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 age parameter (see Parameters). It is well-studied in the literature.
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 | β | 260.798 | -37.939 | 0.533 | 1.238 | -0.572 | -19.953 |
| Li et al. | 2025 | 260.781 | -37.898 | 0.604 | 1.044 | 0.922 | β |
| Almeida et al. | 2025 | 260.781 | -37.898 | β | β | β | β |
| Hunt & Reffert | 2024 | 260.86 | -37.916 | 0.653 | 1.672 | -2.056 | -20.683 |
| Cavallo et al. | 2024 | 260.868 | -37.905 | 0.654 | β | β | β |
| He et al. | 2023 | 260.855 | -37.909 | 0.658 | 1.699 | -2.034 | β |
| Hunt & Reffert | 2023 | 260.86 | -37.916 | 0.653 | 1.672 | -2.056 | -20.683 |
| Just et al. | 2023 | 260.871 | -37.925 | β | β | β | β |
| Dias et al. | 2021 | 260.781 | -37.898 | 0.604 | 1.044 | 0.922 | β |
| SΓ‘nchez et al. | 2020 | 260.858 | -37.9 | β | 1.233 | -1.963 | β |
| Monteiro & Dias | 2019 | 260.88 | -37.925 | β | 1.03 | 0.888 | 3.055 |
| Kharchenko et al. | 2016 | 260.871 | -37.925 | β | β | β | β |
| Dias et al. | 2014 | 260.858 | -37.9 | β | -0.79 | -3.15 | β |
| Kharchenko et al. | 2013 | 260.88 | -37.925 | β | 0.65 | -2.0 | β |
| Kharchenko et al. | 2003 | 260.85 | -37.96 | β | -2.49 | -0.02 | β |
| Dias et al. | 2002 | 260.858 | -37.9 | β | -0.79 | -3.15 | β |
π‘ 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 |
|---|---|---|---|---|---|---|---|---|---|
| Li et al. | 2025 | 1.55 | 1.87 | β | 516 | 0.160 | β | β | β |
| Almeida et al. | 2025 | 1.51 | 1.91 | β | 481 | β | 76 | β | β |
| Hunt & Reffert | 2024 | β | β | β | β | β | 321* | β | β |
| Cavallo et al. | 2024 | 1.47 | 1.64 | β | 129 | 0.280 | β | β | β |
| He et al. | 2023 | 1.45 | 2.00 | β | 32 | β | β | β | β |
| Hunt & Reffert | 2023 | 1.45 | 1.77 | 1.13 | 242 | β | β | β | β |
| Just et al. | 2023 | β | β | β | 126 | β | 60 | β | β |
| Dias et al. | 2021 | 1.51 | 1.91 | β | 481 | 0.188 | β | β | β |
| Monteiro & Dias | 2019 | 1.72 | 1.46 | β | 612 | 0.020 | β | β | β |
| Kharchenko et al. | 2016 | 0.93 | 0.58 | β | 126 | β | β | β | β |
| Kharchenko et al. | 2013 | 0.93 | 0.58 | β | 126 | β | β | β | β |
| Kharchenko et al. | 2003 | 0.71 | 0.62 | β | β | β | β | β | β |
| Dias et al. | 2002 | 0.71 | 0.62 | β | β | β | β | β | β |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Almeida et al. (2025)
Mass determination: worst fit. Isochrone match: good fit.
Cavallo et al. (2024)
Gold sample.