Saurer 2
(MWSC 1489; FSR 1386)
0.82
UTI
0.8
CN
1.0
Cdens
0.75
CC3
0.79
Clit
1.0
Cdup
Radius (P>50% members)
1.4 [arcmin]
- CN 0.8 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.79 Well-studied
- Cdup 1.0 Unique
Overview
Saurer 2 is a rich, very 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, near-solar metallicity, old cluster, but with a large variance across recent sources for the age parameter (see Parameters). It is well-studied in the literature.
Very distant
High extinction
Massive
Near-solar metallicity
Old
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 126.359 | -39.632 | 0.141 | -2.973 | 4.605 | 87.709 |
| Hu & Soubiran | 2025 | 126.351 | -39.642 | â | â | â | â |
| Hunt & Reffert | 2024 | 126.363 | -39.635 | 0.118 | -2.99 | 4.58 | 87.721 |
| Cavallo et al. | 2024 | 126.351 | -39.642 | 0.122 | â | â | â |
| Hunt & Reffert | 2023 | 126.363 | -39.635 | 0.118 | -2.99 | 4.58 | 87.721 |
| Just et al. | 2023 | 126.354 | -39.637 | â | â | â | â |
| Cantat-Gaudin et al. | 2020 | 126.366 | -39.64 | 0.109 | -2.969 | 4.567 | â |
| Cantat-Gaudin & Anders | 2020 | 126.366 | -39.64 | 0.109 | -2.969 | 4.567 | â |
| Soubiran et al. | 2018 | 126.366 | -39.64 | â | â | â | 84.59 |
| Bica et al. | 2019 | 126.357 | -39.621 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 126.366 | -39.64 | 0.109 | -2.969 | 4.567 | â |
| Kharchenko et al. | 2016 | 126.354 | -39.637 | â | â | â | â |
| Kharchenko et al. | 2013 | 126.36 | -39.64 | â | -6.62 | 8.13 | â |
| van den Bergh | 2006 | 126.375 | -39.633 | â | â | â | â |
| Dias et al. | 2002 | 126.367 | -39.634 | â | -1.01 | 3.64 | 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 | -0.450* | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 2393* | â | â |
| Cavallo et al. | 2024 | 6.58 | 3.69 | â | 1950 | -0.160 | â | â | â |
| Hunt & Reffert | 2023 | 6.26 | 4.12 | 2.71 | 394 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 1778 | â | 731 | â | â |
| Cantat-Gaudin et al. | 2020 | 6.43 | 3.72 | â | 1622 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 7.26 | â | â | â | â | â | â | â |
| Soubiran et al. | 2018 | 7.26 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 7.26 | â | â | â | â | â | â | â |
| Kharchenko et al. | 2016 | 6.02 | 3.87 | â | 1778 | â | â | â | â |
| Kharchenko et al. | 2013 | 6.02 | 3.87 | â | 1778 | â | â | â | â |
| van den Bergh | 2006 | 4.70 | 3.84 | â | 2512 | â | â | â | â |
| Dias et al. | 2002 | 6.60 | 3.32 | â | 1995 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Gold sample.