Ruprecht 119
(MWSC 2413; OCL 963; ESO 226 10)
- CN 0.75 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
(*): The parallax distance estimate (~2.21 kpc) differs significantly from the median photometric distance (~1.69 kpc).
Note: This object shares a small percentage of members with a later reported entry. See table with shared members information.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | – | 247.012 | -51.495 | 0.452 | -1.349 | -3.416 | -46.702 |
| Almeida et al. | 2025 | 247.042 | -51.504 | – | – | – | – |
| Hunt & Reffert | 2024 | 247.003 | -51.496 | 0.455 | -1.407 | -3.416 | -45.258 |
| Cavallo et al. | 2024 | 247.02 | -51.485 | 0.455 | – | – | – |
| Hunt & Reffert | 2023 | 247.003 | -51.496 | 0.455 | -1.407 | -3.416 | -45.258 |
| Just et al. | 2023 | 247.039 | -51.509 | – | – | – | – |
| Jaehnig et al. | 2021 | 247.037 | -51.497 | 0.469 | -1.298 | -3.426 | – |
| Rain et al. | 2021 | 247.039 | -51.5 | 0.433 | -1.3 | -3.413 | – |
| Dias et al. | 2021 | 247.042 | -51.504 | 0.439 | -1.314 | -3.424 | – |
| Cantat-Gaudin et al. | 2020 | 247.039 | -51.5 | 0.433 | -1.3 | -3.413 | – |
| Soubiran et al. | 2018 | 247.039 | -51.5 | – | – | – | -39.38 |
| Bica et al. | 2019 | 247.034 | -51.505 | – | – | – | – |
| Cantat-Gaudin et al. | 2018 | 247.039 | -51.5 | 0.433 | -1.3 | -3.413 | – |
| Loktin & Popova | 2017 | 247.065 | -51.501 | – | -3.809 | -8.03 | -11.2 |
| Kharchenko et al. | 2016 | 247.039 | -51.509 | – | – | – | – |
| Kharchenko et al. | 2013 | 247.05 | -51.51 | – | -2.11 | -0.56 | -11.2 |
| Piskunov et al. | 2008 | 247.057 | -51.505 | – | – | – | – |
| Kharchenko et al. | 2005 | 247.06 | -51.5 | – | -2.17 | -0.35 | – |
| Kharchenko et al. | 2003 | 247.03 | -51.52 | – | -2.42 | -0.96 | – |
| Dias et al. | 2002 | 247.062 | -51.5 | – | -2.13 | -3.42 | -11.21 |
| Dambis | 1999 | 247.062 | -51.5 | – | – | – | – |
💡 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 |
|---|---|---|---|---|---|---|---|---|---|
| Almeida et al. | 2025 | 1.90 | 1.86 | – | 101 | – | 369 | – | – |
| Hunt & Reffert | 2024 | – | – | – | – | – | 1231* | – | – |
| Cavallo et al. | 2024 | 1.69 | 1.87 | – | 263 | 0.220 | – | – | – |
| Hunt & Reffert | 2023 | 1.99 | 1.91 | 2.15 | 48 | – | – | – | – |
| Just et al. | 2023 | – | – | – | 272 | – | 72 | – | – |
| Jaehnig et al. | 2021 | 2.13* | – | – | – | – | – | – | – |
| Rain et al. | 2021 | 2.16 | 1.77 | – | 7 | – | – | – | 0 |
| Dias et al. | 2021 | 1.90 | 1.86 | – | 101 | 0.183 | – | – | – |
| Cantat-Gaudin et al. | 2020 | 2.23 | 1.49 | – | 48 | – | – | – | – |
| Soubiran et al. | 2018 | 2.16 | – | – | – | – | – | – | – |
| Cantat-Gaudin et al. | 2018 | 2.16 | – | – | – | – | – | – | – |
| Loktin & Popova | 2017 | 1.00 | 1.71 | – | 10 | – | – | – | – |
| Kharchenko et al. | 2016 | 1.10 | 1.77 | – | 272 | – | – | – | – |
| Kharchenko et al. | 2013 | 1.10 | 1.77 | – | 272 | – | – | – | – |
| Piskunov et al. | 2008 | 0.96 | 1.77 | – | 27 | – | – | – | – |
| Kharchenko et al. | 2005 | 0.96 | 1.77 | – | 27 | – | – | – | – |
| Kharchenko et al. | 2003 | 0.96 | 1.55 | – | – | – | – | – | – |
| Dias et al. | 2002 | 0.96 | 1.77 | – | 7 | – | – | – | – |
| Dambis | 1999 | 0.95 | 1.73 | – | 45 | – | – | – | – |
💡 Note: The parameters are sometimes
transformed from their original values to match the format of the
columns shown here, see FAQ.
The columns DAv, Bfr, BSS correspond to differential
extinction, binary fraction, and blue stragglers, respectively.
BSS values can be listed as fractions or integers.
(*): 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.