Ruprecht 35
(VDBH 10; MWSC 1333; OCL 689; vdBergh-Hagen 10; ESO 429 18)
0.89
UTI
0.7
CN
1.0
Cdens
0.75
CC3
1.0
Clit
1.0
Cdup
Radius (P>50% members)
1.9 [arcmin]
- CN 0.7 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
Ruprecht 35 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a moderate 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 absorption and age parameters (see Parameters). It is very well-studied in the literature.
Distant
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 | 116.551 | -31.28 | 0.255 | -2.259 | 3.179 | â |
| Li et al. | 2025 | 116.548 | -31.278 | 0.243 | -2.256 | 3.136 | â |
| Almeida et al. | 2025 | 116.545 | -31.274 | â | â | â | â |
| Hunt & Reffert | 2024 | 116.553 | -31.279 | 0.251 | -2.262 | 3.203 | â |
| Cavallo et al. | 2024 | 116.549 | -31.281 | 0.253 | â | â | â |
| Hunt & Reffert | 2023 | 116.553 | -31.279 | 0.251 | -2.262 | 3.203 | â |
| Almeida et al. | 2023 | 116.555 | -31.276 | â | â | â | â |
| Just et al. | 2023 | 116.548 | -31.28 | â | â | â | â |
| Dias et al. | 2021 | 116.545 | -31.274 | 0.244 | -2.256 | 3.133 | â |
| Cantat-Gaudin et al. | 2020 | 116.548 | -31.278 | 0.243 | -2.256 | 3.136 | â |
| Cantat-Gaudin & Anders | 2020 | 116.548 | -31.278 | 0.243 | -2.256 | 3.136 | â |
| Soubiran et al. | 2018 | 116.548 | -31.278 | â | â | â | 91.27 |
| Bica et al. | 2019 | 116.553 | -31.28 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 116.548 | -31.278 | 0.243 | -2.256 | 3.136 | â |
| Kharchenko et al. | 2016 | 116.548 | -31.28 | â | â | â | â |
| Dias et al. | 2014 | 116.558 | -31.28 | â | -1.66 | 3.24 | â |
| Kharchenko et al. | 2013 | 116.553 | -31.283 | â | -0.66 | 2.1 | â |
| Dias et al. | 2002 | 116.558 | -31.28 | â | -1.66 | 3.24 | 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 |
|---|---|---|---|---|---|---|---|---|---|
| Li et al. | 2025 | 1.64 | 0.17 | â | 2954 | -0.128 | â | â | â |
| Almeida et al. | 2025 | 3.02 | 1.77 | â | 153 | â | 292 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 787* | â | â |
| Cavallo et al. | 2024 | 3.42 | 1.92 | â | 35 | -0.030 | â | â | â |
| Hunt & Reffert | 2023 | 3.57 | 1.81 | 2.04 | 26 | â | â | â | â |
| Almeida et al. | 2023 | 3.25 | 1.95 | â | 25 | -0.153 | 450* | 0.59 | â |
| Just et al. | 2023 | â | â | â | 275 | â | 973 | â | â |
| Dias et al. | 2021 | 3.02 | 1.77 | â | 153 | -0.136 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 3.96 | 1.49 | â | 55 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 3.68 | â | â | â | â | â | â | â |
| Soubiran et al. | 2018 | 3.68 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 3.68 | â | â | â | â | â | â | â |
| Kharchenko et al. | 2016 | 3.86 | 2.58 | â | 275 | â | â | â | â |
| Kharchenko et al. | 2013 | 3.86 | 2.58 | â | 275 | â | â | â | â |
| Dias et al. | 2002 | 3.91 | 1.40 | â | 398 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


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