Loden 189
(MWSC 1858)
0.43
UTI
0.25
CN
0.14
Cdens
0.38
CC3
0.7
Clit
1.0
Cdup
Radius (P>50% members)
16.0 [arcmin]
- CN 0.25 Poorly populated
- Cdens 0.14 Very loose
- CC3 0.38 Low quality
- Clit 0.7 Moderately studied
- Cdup 1.0 Unique
Overview
Loden 189 is a poorly populated, very loose object of low C3 quality. Its parallax locates it at a relatively close* distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It is moderately studied in the literature.
(*): The parallax distance estimate (~1.31 kpc) differs significantly from the median photometric distance (~0.82 kpc).
Close
Low extinction
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 | 162.552 | -56.331 | 0.766 | -7.544 | 3.301 | 3.032 |
| Hu & Soubiran | 2025 | 162.514 | -56.327 | â | â | â | â |
| Hunt & Reffert | 2024 | 162.73 | -56.33 | 0.765 | -7.505 | 3.268 | 6.539 |
| Cavallo et al. | 2024 | 162.515 | -56.327 | 0.768 | â | â | â |
| Hunt & Reffert | 2023 | 162.73 | -56.33 | 0.765 | -7.505 | 3.268 | 6.539 |
| Just et al. | 2023 | 162.609 | -56.416 | â | â | â | â |
| Loktin & Popova | 2017 | 162.495 | -56.399 | â | -4.84 | -0.93 | 12.0 |
| Kharchenko et al. | 2016 | 162.609 | -56.416 | â | â | â | â |
| Dias et al. | 2014 | 162.5 | -56.4 | â | -4.84 | -0.93 | 49.53 |
| Kharchenko et al. | 2013 | 162.615 | -56.42 | â | -5.9 | 2.03 | 12.0 |
| Piskunov et al. | 2008 | 162.577 | -56.421 | â | â | â | â |
| Piskunov et al. | 2007 | 162.577 | -56.421 | â | â | â | â |
| Kharchenko et al. | 2005 | 162.58 | -56.42 | â | -5.73 | 2.91 | 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 |
|---|---|---|---|---|---|---|---|---|---|
| Hu & Soubiran | 2025 | â | â | â | â | -0.310* | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 79* | â | â |
| Cavallo et al. | 2024 | 1.22 | 0.33 | â | 912 | 0.020 | â | â | â |
| Hunt & Reffert | 2023 | 1.27 | 0.24 | 0.51 | 676 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 98 | â | 75 | â | â |
| Loktin & Popova | 2017 | 1.14 | 0.40 | â | 437 | â | â | â | â |
| Kharchenko et al. | 2016 | 0.82 | 0.32 | â | 98 | â | â | â | â |
| Kharchenko et al. | 2013 | 0.82 | 0.32 | â | 98 | 0.202 | â | â | â |
| Piskunov et al. | 2008 | 0.72 | 0.40 | â | 437 | â | 184* | â | â |
| Piskunov et al. | 2007 | 0.72 | 0.40 | â | 437 | â | 51 | â | â |
| Kharchenko et al. | 2005 | 0.72 | 0.40 | â | 437 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Gold sample.