Ruprecht 56
(MWSC 1452; OCL 730; ESO 312 01)
0.38
UTI
0.0
CN
0.02
Cdens
0.38
CC3
0.75
Clit
1.0
Cdup
Radius (P>50% members)
7.9 [arcmin]
- CN 0.0 Sparse
- Cdens 0.02 Very loose
- CC3 0.38 Low quality
- Clit 0.75 Well-studied
- Cdup 1.0 Unique
Overview
Ruprecht 56 is a sparse, very loose object of low C3 quality. Its parallax locates it at a large* distance, below the mid-plane, affected by low extinction. It is catalogued as a low-mass, near-solar metallicity, intermediate-age cluster (see Parameters). It is well-studied in the literature.
(*): The parallax distance estimate (~5.98 kpc) differs significantly from the median photometric distance (~0.43 kpc).
Very close
Low extinction
Low mass
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 | 123.023 | -40.514 | 0.167 | -2.42 | 3.281 | 55.011 |
| Hunt & Reffert | 2024 | 122.958 | -40.496 | 0.151 | -2.427 | 3.262 | 94.417 |
| Cavallo et al. | 2024 | 122.895 | -40.514 | 0.156 | â | â | â |
| Hunt & Reffert | 2023 | 122.958 | -40.496 | 0.151 | -2.427 | 3.262 | 94.417 |
| Just et al. | 2023 | 123.16 | -40.482 | â | â | â | â |
| Bica et al. | 2019 | 123.14 | -40.464 | â | â | â | â |
| Kharchenko et al. | 2016 | 123.16 | -40.482 | â | â | â | â |
| Dias et al. | 2014 | 123.138 | -40.467 | â | -2.48 | 4.58 | â |
| Kharchenko et al. | 2013 | 123.165 | -40.485 | â | -9.4 | 4.8 | â |
| Piskunov et al. | 2008 | 123.129 | -40.47 | â | â | â | â |
| Piskunov et al. | 2007 | 123.129 | -40.47 | â | â | â | â |
| Kharchenko et al. | 2005 | 123.13 | -40.47 | â | -9.71 | 5.75 | â |
| Kharchenko et al. | 2003 | 123.16 | -40.49 | â | -9.84 | 5.97 | â |
| Dias et al. | 2002 | 123.138 | -40.467 | â | -2.48 | 4.58 | 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 |
|---|---|---|---|---|---|---|---|---|---|
| Hunt & Reffert | 2024 | â | â | â | â | â | 403* | â | â |
| Cavallo et al. | 2024 | 3.82 | 2.97 | â | 135 | 0.060 | â | â | â |
| Hunt & Reffert | 2023 | 5.86 | 2.93 | 1.73 | 121 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 556 | â | 10 | â | â |
| Kharchenko et al. | 2016 | 0.43 | 0.38 | â | 556 | â | â | â | â |
| Kharchenko et al. | 2013 | 0.43 | 0.38 | â | 556 | â | â | â | â |
| Piskunov et al. | 2008 | 0.41 | 0.37 | â | 501 | â | 17* | â | â |
| Piskunov et al. | 2007 | 0.41 | 0.37 | â | 501 | â | 4 | â | â |
| Kharchenko et al. | 2005 | 0.41 | 0.37 | â | 501 | â | â | â | â |
| Kharchenko et al. | 2003 | 0.83 | 0.31 | â | â | â | â | â | â |
| Dias et al. | 2002 | 0.41 | 0.37 | â | 501 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Gold sample.