Ruprecht 89
(MWSC 1808; OCL 812; ESO 127 21)
0.26
UTI
0.0
CN
0.2
Cdens
0.12
CC3
0.5
Clit
1.0
Cdup
Radius (P>50% members)
5.6 [arcmin]
- CN 0.0 Sparse
- Cdens 0.2 Very loose
- CC3 0.12 Very low quality
- Clit 0.5 Moderately studied
- Cdup 1.0 Unique
Overview
Ruprecht 89 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a moderate* distance, near 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 (~2.47 kpc) differs significantly from the median photometric distance (~0.75 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 | 157.134 | -58.164 | 0.405 | -7.066 | 2.571 | â |
| Just et al. | 2023 | 157.102 | -58.131 | â | â | â | â |
| Bica et al. | 2019 | 157.109 | -58.18 | â | â | â | â |
| Kharchenko et al. | 2016 | 157.102 | -58.131 | â | â | â | â |
| Dias et al. | 2014 | 157.108 | -58.183 | â | -4.12 | 1.3 | â |
| Kharchenko et al. | 2013 | 157.107 | -58.135 | â | -3.75 | 5.13 | â |
| Piskunov et al. | 2008 | 157.116 | -58.136 | â | â | â | â |
| Kharchenko et al. | 2005 | 157.11 | -58.14 | â | -6.82 | 4.36 | â |
| Kharchenko et al. | 2003 | 157.06 | -58.13 | â | -5.86 | 4.04 | 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 | 955 | â | 10 | â | â |
| Kharchenko et al. | 2016 | 0.75 | 0.12 | â | 955 | â | â | â | â |
| Kharchenko et al. | 2013 | 0.75 | 0.12 | â | 955 | â | â | â | â |
| Piskunov et al. | 2008 | 0.75 | 0.12 | â | 955 | â | â | â | â |
| Kharchenko et al. | 2005 | 0.75 | 0.12 | â | 955 | â | â | â | â |
| Kharchenko et al. | 2003 | 0.91 | 0.31 | â | â | â | â | â | â |
