Saurer 6
(MWSC 3193; FSR 0180)
0.33
UTI
0.0
CN
0.01
Cdens
0.62
CC3
0.5
Clit
1.0
Cdup
Stellar density (N50/rad)
0.0 [N/pc2]
- CN 0.0 Sparse
- Cdens 0.01 Very loose
- CC3 0.62 Intermediate quality
- Clit 0.5 Moderately studied
- Cdup 1.0 Unique
Overview
Saurer 6 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a large distance, above the mid-plane, affected by moderate extinction. It is catalogued as a massive, near-solar metallicity, old cluster (see Parameters). It is moderately studied in the literature.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 297.768 | 32.23 | 0.124 | -2.759 | -4.505 | -57.162 |
| He et al. | 2023 | 297.755 | 32.244 | 0.073 | -2.548 | -4.057 | -80.41 |
| Just et al. | 2023 | 297.753 | 32.231 | â | â | â | â |
| Perren et al. | 2022 | 297.75 | 32.25 | â | â | â | â |
| Bica et al. | 2019 | 297.769 | 32.238 | â | â | â | â |
| Kharchenko et al. | 2016 | 297.753 | 32.231 | â | â | â | â |
| Dias et al. | 2014 | 297.758 | 32.243 | â | -1.84 | -1.38 | â |
| Kharchenko et al. | 2013 | 297.759 | 32.233 | â | -3.95 | -0.61 | â |
| van den Bergh | 2006 | 297.75 | 32.25 | â | â | â | â |
| Dias et al. | 2002 | 297.758 | 32.243 | â | -2.08 | -1.56 | 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 | 8.955 | 2.65 | â | 1585 | -0.110 | 3664 | 0.52 | â |
| He et al. | 2023 | 8.71 | 2.90 | â | 1259 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 1585 | â | 2128 | â | â |
| Perren et al. | 2022 | 9.20 | 2.91 | â | 1380 | -0.110 | 5200 | 0.52 | â |
| Kharchenko et al. | 2016 | 7.33 | 2.65 | â | 1585 | â | â | â | â |
| Kharchenko et al. | 2013 | 7.33 | 2.65 | â | 1585 | â | â | â | â |
| van den Bergh | 2006 | 9.33 | 2.39 | â | 1950 | â | â | â | â |
| Dias et al. | 2002 | 9.33 | 2.39 | â | 1950 | â | â | â | â |
MOCA
