Ruprecht 166
(OCL 899; ESO 096 11; MWSC 2119)
0.48
UTI
0.26
CN
0.65
Cdens
0.75
CC3
0.38
Clit
1.0
Cdup
Radius (P>50% members)
1.2 [arcmin]
- CN 0.26 Poorly populated
- Cdens 0.65 Moderately dense
- CC3 0.75 High quality
- Clit 0.38 Poorly studied
- Cdup 1.0 Unique
Overview
Ruprecht 166 is a poorly populated, moderately dense object of high C3 quality. Its parallax locates it at a large* distance, below the mid-plane, affected by high extinction. It is catalogued as a massive, metal-poor, intermediate-age cluster (see Parameters). It is poorly studied in the literature.
(*): The parallax distance estimate (~8.12 kpc) differs significantly from the median photometric distance (~5.11 kpc).
Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.
Very distant
High extinction
Massive
Metal-poor
Intermediate age
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 201.416 | -63.459 | 0.123 | -6.938 | -1.134 | -38.099 |
| Hunt & Reffert | 2024 | 201.399 | -63.459 | 0.119 | -6.948 | -1.136 | -33.78 |
| Cavallo et al. | 2024 | 201.431 | -63.451 | 0.118 | â | â | â |
| Hunt & Reffert | 2023 | 201.399 | -63.459 | 0.119 | -6.948 | -1.136 | -33.78 |
| Bica et al. | 2019 | 201.403 | -63.449 | â | â | â | â |
| Dias et al. | 2014 | 201.413 | -63.467 | â | -4.01 | -2.24 | â |
| Dias et al. | 2002 | 201.412 | -63.467 | â | -3.93 | -2.32 | 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 |
|---|---|---|---|---|---|---|---|---|---|
| Hunt & Reffert | 2024 | â | â | â | â | â | 1606* | â | â |
| Cavallo et al. | 2024 | 2.55 | 2.99 | â | 331 | -0.840 | â | â | â |
| Hunt & Reffert | 2023 | 7.67 | 3.10 | 2.41 | 11 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Gold sample.