Ruprecht 59
(OCL 717; ESO 370 07; MWSC 1472)
0.44
UTI
0.32
CN
0.06
Cdens
0.75
CC3
0.54
Clit
1.0
Cdup
Nm (P>50%)
32
Core radius and density
4.3 [pc], 0.3 [pc-2]
- CN 0.32 Poorly populated
- Cdens 0.06 Very loose
- CC3 0.75 High quality
- Clit 0.54 Moderately studied
- Cdup 1.0 Unique
Overview
Ruprecht 59 is a poorly populated, very loose object of high C3 quality. Its parallax locates it at a large* distance, above the mid-plane, affected by low extinction. It is catalogued as a metal-poor, young cluster (see Parameters). It is moderately studied in the literature.
(*): The parallax distance estimate (~6.70 kpc) differs significantly from the median photometric distance (~2.14 kpc).
Note: This object shares a large 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 | 99999â | 124.819 | -34.479 | 0.149 | -2.588 | 3.235 | â |
| Hunt & Reffert | 2024 | 124.826 | -34.482 | 0.15 | -2.579 | 3.238 | â |
| Cavallo et al. | 2024 | 124.834 | -34.463 | 0.15 | â | â | â |
| Hunt & Reffert | 2023 | 124.826 | -34.482 | 0.15 | -2.579 | 3.238 | â |
| Bica et al. | 2019 | 124.821 | -34.48 | â | â | â | â |
| Dias et al. | 2018 | â | â | â | -3.71 | 2.87 | â |
| Loktin & Popova | 2017 | 124.845 | -34.483 | â | -5.159 | 5.656 | 12.5 |
| Sampedro et al. | 2017 | 124.838 | -34.483 | â | -3.86 | 0.3 | â |
| Dias et al. | 2014 | 124.838 | -34.483 | â | -2.37 | 0.36 | â |
| van den Bergh | 2006 | 124.829 | -34.485 | â | â | â | â |
| Dias et al. | 2002 | 124.838 | -34.483 | â | -2.37 | 0.36 | â |
| Lynga | 1987 | 124.791 | -34.461 | â | â | â | 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] | Bfrac | BSS |
|---|---|---|---|---|---|---|---|---|---|
| UCC | 99999â | 2.14 | 0.975 | 0.76 | 45 | -0.790 | 391 | â | â |
| Hunt & Reffert | 2024 | 6.20 | 1.67 | 0.76 | 30 | â | 391(1) | â | â |
| Cavallo et al. | 2024 | 3.25 | 1.99 | â | 37 | -0.790 | â | â | â |
| Hunt & Reffert | 2023 | 6.20 | 1.67 | 0.76 | 30 | â | â | â | â |
| Loktin & Popova | 2017 | 1.03 | 0.28 | â | 77 | â | â | â | â |
| van den Bergh | 2006 | 0.87 | 0.28 | â | 54 | â | â | â | â |
| Dias et al. | 2002 | 0.87 | 0.28 | â | 53 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as open cluster. CMD class: 1.00 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 1.00 (50th percentile).