SAI 16
(MWSC 165)
0.82
UTI
0.72
CN
1.0
Cdens
0.38
CC3
1.0
Clit
1.0
Cdup
Radius (P>50% members)
2.1 [arcmin]
- CN 0.72 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.38 Low quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
SAI 16 is a moderately populated, very dense object of low C3 quality. Its parallax locates it at a large distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, old cluster (see Parameters). It is very well-studied in the literature.
Distant
Moderate extinction
Near-solar metallicity
Old
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 31.377 | 62.267 | 0.181 | -0.796 | -0.388 | -81.657 |
| Hunt & Reffert | 2024 | 31.39 | 62.265 | 0.212 | -0.799 | -0.35 | -56.257 |
| Cavallo et al. | 2024 | 31.308 | 62.304 | 0.219 | â | â | â |
| Hunt & Reffert | 2023 | 31.39 | 62.265 | 0.212 | -0.799 | -0.35 | -56.257 |
| Just et al. | 2023 | 31.4 | 62.263 | â | â | â | â |
| Cantat-Gaudin et al. | 2020 | 31.366 | 62.265 | 0.157 | -0.725 | -0.305 | â |
| Donor et al. | 2020 | 31.413 | 62.265 | â | -0.7 | -0.37 | -61.2 |
| Cantat-Gaudin & Anders | 2020 | 31.366 | 62.265 | 0.157 | -0.725 | -0.305 | â |
| Soubiran et al. | 2018 | 31.366 | 62.265 | â | â | â | -65.59 |
| Bica et al. | 2019 | 31.372 | 62.264 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 31.366 | 62.265 | 0.157 | -0.725 | -0.305 | â |
| Loktin & Popova | 2017 | 31.38 | 62.265 | â | 0.108 | -1.188 | â |
| Kharchenko et al. | 2016 | 31.4 | 62.263 | â | â | â | â |
| Dias et al. | 2014 | 31.375 | 62.265 | â | -1.87 | -0.91 | â |
| Kharchenko et al. | 2013 | 31.413 | 62.265 | â | -0.31 | -1.42 | â |
| Kharchenko et al. | 2012 | 31.413 | 62.265 | â | -0.31 | -1.42 | â |
| Glushkova et al. | 2010 | 31.373 | 62.265 | â | â | â | â |
| Dias et al. | 2002 | 31.375 | 62.265 | â | -1.87 | -0.91 | 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 |
|---|---|---|---|---|---|---|---|---|---|
| Hunt & Reffert | 2024 | â | â | â | â | â | 962* | â | â |
| Cavallo et al. | 2024 | 4.00 | 2.35 | â | 269 | 0.140 | â | â | â |
| Hunt & Reffert | 2023 | 3.89 | 2.54 | 2.29 | 272 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 1413 | â | 366 | â | â |
| Cantat-Gaudin et al. | 2020 | 4.90 | 2.68 | â | 1000 | â | â | â | â |
| Donor et al. | 2020 | â | â | â | â | -0.280 | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 5.37 | â | â | â | â | â | â | â |
| Soubiran et al. | 2018 | 5.37 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 5.37 | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 1.96 | 2.48 | â | 1413 | â | â | â | â |
| Kharchenko et al. | 2016 | 4.74 | 3.10 | â | 1413 | â | â | â | â |
| Kharchenko et al. | 2013 | 4.74 | 3.10 | â | 1413 | â | â | â | â |
| Kharchenko et al. | 2012 | 4.74 | 3.10 | â | 1413 | â | â | â | â |
| Glushkova et al. | 2010 | 7.70 | 2.17 | â | 1413 | â | â | â | â |
| Dias et al. | 2002 | 7.70 | 2.17 | â | 1413 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Bronze sample.