Ruprecht 99
(MWSC 1994; OCL 872; ESO 094 11)
0.27
UTI
0.0
CN
0.01
Cdens
0.62
CC3
0.35
Clit
1.0
Cdup
Nm (P>50%)
18
Core radius and density
6.1 [pc], 0.03 [pc-2]
- CN 0.0 Sparse
- Cdens 0.01 Very loose
- CC3 0.62 Intermediate quality
- Clit 0.35 Poorly studied
- Cdup 1.0 Unique
Overview
Ruprecht 99 is a sparse, very loose object of intermediate 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, intermediate-age cluster (see Parameters). It is poorly studied in the literature.
(*): The parallax distance estimate (~6.72 kpc) differs significantly from the median photometric distance (~0.72 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.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 180.874 | -63.874 | 0.149 | -7.057 | 1.062 | -7.403 |
| Just et al. | 2023 | 180.862 | -63.857 | â | â | â | â |
| Bica et al. | 2019 | 180.822 | -63.868 | â | â | â | â |
| Dias et al. | 2018 | â | â | â | -7.37 | -0.85 | â |
| Dib et al. | 2018 | 180.87 | -63.86 | â | â | â | â |
| Sampedro et al. | 2017 | 180.767 | -63.85 | â | -4.88 | 0.06 | â |
| Joshi et al. | 2016 | 180.87 | -63.86 | â | â | â | â |
| Kharchenko et al. | 2016 | 180.862 | -63.857 | â | â | â | â |
| Dias et al. | 2014 | 180.767 | -63.85 | â | -4.69 | 0.23 | â |
| Kharchenko et al. | 2013 | 180.87 | -63.86 | â | -7.74 | -2.07 | â |
| Piskunov et al. | 2008 | 180.818 | -63.878 | â | â | â | â |
| Kharchenko et al. | 2005 | 180.82 | -63.88 | â | -7.9 | -2.96 | â |
| Dias et al. | 2002 | 180.767 | -63.85 | â | -4.69 | 0.23 | â |
| Lynga | 1987 | 180.777 | -63.813 | 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 | 0.72 | 0.16 | â | 237 | â | 24 | â | â |
| Just et al. | 2023 | â | â | â | 237 | â | 29 | â | â |
| Dib et al. | 2018 | 0.72 | â | â | 237 | â | â | â | â |
| Joshi et al. | 2016 | 0.72 | 0.16 | â | 237 | â | 18 | â | â |
| Kharchenko et al. | 2016 | 0.72 | 0.16 | â | 237 | â | â | â | â |
| Kharchenko et al. | 2013 | 0.72 | 0.16 | â | 237 | â | â | â | â |
| Piskunov et al. | 2008 | 0.66 | 0.16 | â | 1950 | â | â | â | â |
| Kharchenko et al. | 2005 | 0.66 | 0.16 | â | 1950 | â | â | â | â |
| Dias et al. | 2002 | 0.66 | 0.16 | â | 1950 | â | â | â | â |
MOCA
