Ruprecht 46
(MWSC 1418; OCL 637; ESO 561 08)
0.23
UTI
0.0
CN
0.14
Cdens
0.25
CC3
0.38
Clit
1.0
Cdup
Radius (P>50% members)
6.0 [arcmin]
- CN 0.0 Sparse
- Cdens 0.14 Very loose
- CC3 0.25 Low quality
- Clit 0.38 Poorly studied
- Cdup 1.0 Unique
Overview
Ruprecht 46 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate* distance, above the mid-plane, affected by low extinction. It is catalogued as a low-mass, near-solar metallicity, intermediate-age cluster (see Parameters). It is poorly studied in the literature.
(*): The parallax distance estimate (~3.17 kpc) differs significantly from the median photometric distance (~1.11 kpc).
â ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.
Relatively 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 | 120.542 | -19.454 | 0.315 | -1.087 | 0.226 | â |
| Just et al. | 2023 | 120.541 | -19.462 | â | â | â | â |
| Bica et al. | 2019 | 120.542 | -19.461 | â | â | â | â |
| Kharchenko et al. | 2016 | 120.541 | -19.462 | â | â | â | â |
| Kharchenko et al. | 2013 | 120.547 | -19.465 | â | -6.78 | 1.83 | â |
| van den Bergh | 2006 | 120.542 | -19.465 | â | â | â | â |
| Chen et al. | 2003 | 120.533 | -19.466 | 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] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| Just et al. | 2023 | â | â | â | 141 | â | 23 | â | â |
| Kharchenko et al. | 2016 | 1.47 | 1.62 | â | 141 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.47 | 1.62 | â | 141 | â | â | â | â |
| van den Bergh | 2006 | 0.75 | 0.22 | â | 3981 | â | â | â | â |
| Chen et al. | 2003 | 0.75 | 0.22 | â | 3980 | -0.040* | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Cantat-Gaudin et al. (2020)
Density enhancement without meaningful CMD features; likely not a real cluster. More details in Appendix A of the article.
Dias et al. (2002)
Asterism (Carraro, G.; Patat, F. 1995, MNRAS 276, 563)