Ruprecht 134
(VDBH 252; MWSC 2730; OCL 4; vdBergh-Hagen 252; ESO 456 01)
0.96
UTI
0.81
CN
1.0
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
Stellar density (N50/rad)
37.2 [N/pc2]
- CN 0.81 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
π₯ Members
π Colab
π¬ Bayestar19
MOCA
π CDS
π Simbad
π CDS (Ξ±, Ξ΄)
π Simbad (Ξ±, Ξ΄)
MOCA
π CDS
π Simbad
π CDS (Ξ±, Ξ΄)
π Simbad (Ξ±, Ξ΄)
Overview
Ruprecht 134 is a rich, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as a massive, near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the age, metallicity, and mass parameters (see Parameters). It is very well-studied in the literature.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999β | 268.184 | -29.534 | 0.399 | -1.613 | -2.444 | -41.907 |
| Li et al. | 2025 | 268.184 | -29.537 | 0.391 | -1.653 | -2.432 | β |
| Hu & Soubiran | 2025 | 268.177 | -29.53 | β | β | β | β |
| Almeida et al. | 2025 | 268.186 | -29.529 | β | β | β | β |
| Hunt & Reffert | 2024 | 268.175 | -29.535 | 0.392 | -1.607 | -2.441 | -49.743 |
| Cavallo et al. | 2024 | 268.177 | -29.53 | 0.392 | β | β | β |
| Hunt & Reffert | 2023 | 268.175 | -29.535 | 0.392 | -1.607 | -2.441 | -49.743 |
| Just et al. | 2023 | 268.171 | -29.551 | β | β | β | β |
| Dias et al. | 2021 | 268.186 | -29.529 | 0.39 | -1.651 | -2.437 | -42.294 |
| Cantat-Gaudin et al. | 2020 | 268.184 | -29.537 | 0.391 | -1.653 | -2.432 | β |
| SΓ‘nchez et al. | 2020 | 268.179 | -29.55 | β | -1.564 | -2.385 | β |
| Cantat-Gaudin & Anders | 2020 | 268.184 | -29.537 | 0.391 | -1.653 | -2.432 | β |
| Soubiran et al. | 2018 | 268.184 | -29.537 | β | β | β | -42.19 |
| Bica et al. | 2019 | 268.176 | -29.549 | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 268.184 | -29.537 | 0.391 | -1.653 | -2.432 | β |
| Kharchenko et al. | 2016 | 268.171 | -29.551 | β | β | β | β |
| Dias et al. | 2014 | 268.179 | -29.55 | β | -1.03 | -2.25 | β |
| Kharchenko et al. | 2013 | 268.179 | -29.55 | β | -0.28 | 0.56 | β |
| Dias et al. | 2002 | 268.179 | -29.55 | β | -0.98 | -2.22 | 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] | Bfrac | BSS |
|---|---|---|---|---|---|---|---|---|---|
| UCC | 99999β | 2.38 | 2.47 | 1.67 | 687 | -0.141 | 3886 | β | β |
| Li et al. | 2025 | 2.15 | 2.04 | β | 1171 | -0.141 | β | β | β |
| Hu & Soubiran | 2025 | β | β | β | β | -0.140(5) | β | β | β |
| Almeida et al. | 2025 | 2.21 | 1.77 | β | 1380 | β | 347 | β | β |
| Hunt & Reffert | 2024 | β | β | β | β | β | 3886(1) | β | β |
| Cavallo et al. | 2024 | 2.32 | 2.53 | β | 1445 | -1.180 | β | β | β |
| Hunt & Reffert | 2023 | 2.41 | 2.47 | 1.67 | 203 | β | β | β | β |
| Just et al. | 2023 | β | β | β | 76 | β | 105925 | β | β |
| Dias et al. | 2021 | 2.21 | 1.77 | β | 1380 | 0.106 | β | β | β |
| Cantat-Gaudin et al. | 2020 | 2.25 | 1.15 | β | 1660 | β | β | β | β |
| Cantat-Gaudin & Anders | 2020 | 2.38 | β | β | β | β | β | β | β |
| Soubiran et al. | 2018 | 2.38 | β | β | β | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 2.38 | β | β | β | β | β | β | β |
| Kharchenko et al. | 2016 | 6.66 | 2.71 | β | 76 | β | β | β | β |
| Kharchenko et al. | 2013 | 6.66 | 2.71 | β | 76 | β | β | β | β |
| Dias et al. | 2002 | 6.66 | 2.71 | β | 76 | β | β | β | β |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
Almeida et al. (2025)
Mass determination: worst fit. Isochrone match: intermediate fit.
Cavallo et al. (2024)
Gold sample.