Patchick 89
(DSH J1959.5+4918; DC 6)
0.55
UTI
0.73
CN
0.76
Cdens
0.75
CC3
0.26
Clit
1.0
Cdup
Nm (P>50%)
96
Core radius and density
1.7 [pc], 3.8 [pc-2]
- CN 0.73 Moderately populated
- Cdens 0.76 Dense
- CC3 0.75 High quality
- Clit 0.26 Poorly studied
- Cdup 1.0 Unique
Overview
Patchick 89 is a moderately populated, dense object of high C3 quality. Its parallax locates it at a large* distance, well above the mid-plane, affected by low extinction. It is catalogued as a metal-poor, old cluster, but with a large variance across recent sources for the age parameter (see Parameters). It is poorly studied in the literature.
(*): The parallax distance estimate (~7.61 kpc) differs significantly from the median photometric distance (~4.58 kpc).
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 299.882 | 49.314 | 0.131 | -2.996 | -2.303 | -53.154 |
| Hunt & Reffert | 2024 | 299.886 | 49.313 | 0.101 | -3.018 | -2.325 | -53.136 |
| Cavallo et al. | 2024 | 299.891 | 49.304 | 0.114 | â | â | â |
| Hunt & Reffert | 2023 | 299.886 | 49.313 | 0.101 | -3.018 | -2.325 | -53.136 |
| Bica et al. | 2019 | 299.882 | 49.31 | â | â | â | â |
| Sampedro et al. | 2017 | 299.887 | 49.314 | â | 1.39 | -3.92 | â |
| Tadross | 2014 | 299.887 | 49.312 | â | â | â | â |
| Bukowiecki et al. | 2011 | 299.867 | 49.313 | â | â | â | â |
| Kronberger et al. | 2006 | 299.887 | 49.312 | â | â | â | â |
| Dias et al. | 2002 | 299.887 | 49.314 | â | 4.55 | -5.38 | 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 | 4.585 | 0.835 | 1.87 | 1920 | -0.810 | 104 | â | â |
| Hunt & Reffert | 2024 | 8.40 | 0.80 | 1.87 | 570 | â | 180(1) | â | â |
| Cavallo et al. | 2024 | 6.52 | 0.87 | â | 4467 | -0.810 | â | â | â |
| Hunt & Reffert | 2023 | 8.41 | 0.80 | 1.87 | 570 | â | â | â | â |
| Tadross | 2014 | 2.65 | 0.66 | â | 1600 | â | â | â | â |
| Bukowiecki et al. | 2012 | â | â | â | â | â | 29 | â | â |
| Bukowiecki et al. | 2011 | 1.85(1) | 1.01 | â | 2239 | â | â | â | â |
| Dias et al. | 2002 | 1.84 | 1.04 | â | 2239 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Cavallo et al. (2024)
Silver sample.
Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.10 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.10 (50th percentile).
Bica et al. (2019)
Asterisms and cluster alikes by B. Alessi reported in DAML02.