Ruprecht 116
(MWSC 2393)
0.28
UTI
0.0
CN
0.03
Cdens
0.38
CC3
0.5
Clit
1.0
Cdup
Radius (P>50% members)
7.5 [arcmin]
- CN 0.0 Sparse
- Cdens 0.03 Very loose
- CC3 0.38 Low quality
- Clit 0.5 Moderately studied
- Cdup 1.0 Unique
Overview
Ruprecht 116 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate* distance, below the mid-plane, affected by low extinction. It is catalogued as a low-mass, intermediate-age cluster (see Parameters). It is moderately studied in the literature.
(*): The parallax distance estimate (~4.03 kpc) differs significantly from the median photometric distance (~0.90 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.
Close
Low extinction
Low mass
Intermediate age
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 245.851 | -52.027 | 0.248 | -1.964 | -1.484 | â |
| Just et al. | 2023 | 245.839 | -52.0 | â | â | â | â |
| Kharchenko et al. | 2016 | 245.839 | -52.0 | â | â | â | â |
| Dias et al. | 2014 | 245.833 | -52.0 | â | -0.49 | -5.68 | â |
| Kharchenko et al. | 2013 | 245.85 | -52.0 | â | -3.23 | -3.95 | â |
| Piskunov et al. | 2008 | 245.823 | -52.002 | â | â | â | â |
| Kharchenko et al. | 2005 | 245.83 | -52.0 | â | -2.1 | -4.86 | â |
| Kharchenko et al. | 2003 | 245.89 | -52.0 | â | -1.67 | -4.56 | â |
| Dias et al. | 2002 | 245.833 | -52.0 | â | -1.1 | -5.97 | 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 | 891 | â | 37 | â | â |
| Kharchenko et al. | 2016 | 0.90 | 0.42 | â | 891 | â | â | â | â |
| Kharchenko et al. | 2013 | 0.90 | 0.42 | â | 891 | â | â | â | â |
| Piskunov et al. | 2008 | 0.90 | 0.31 | â | 891 | â | â | â | â |
| Kharchenko et al. | 2005 | 0.90 | 0.31 | â | 891 | â | â | â | â |
| Kharchenko et al. | 2003 | 0.67 | 0.31 | â | â | â | â | â | â |
| Dias et al. | 2002 | 0.90 | 0.31 | â | 891 | â | â | â | â |
