Schuster 1
(MWSC 1756; C1002-556; FSR 1523)
0.54
UTI
0.0
CN
0.94
Cdens
0.62
CC3
0.56
Clit
1.0
Cdup
Stellar density (N50/rad)
4.7 [N/pc2]
- CN 0.0 Sparse
- Cdens 0.94 Very dense
- CC3 0.62 Intermediate quality
- Clit 0.56 Moderately studied
- Cdup 1.0 Unique
Overview
Schuster 1 is a sparse, very dense object of intermediate C3 quality. Its parallax locates it at a large distance, near the mid-plane, affected by high extinction. It is catalogued as a very young 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 | 151.154 | -55.855 | 0.154 | -5.242 | 3.6 | 25.939 |
| Celli et al. | 2024 | 151.159 | -55.857 | â | â | â | â |
| Just et al. | 2023 | 151.145 | -55.854 | â | â | â | â |
| Cantat-Gaudin et al. | 2020 | 151.159 | -55.857 | 0.139 | -5.102 | 3.768 | â |
| Cantat-Gaudin & Anders | 2020 | 151.159 | -55.857 | 0.139 | -5.102 | 3.768 | â |
| Soubiran et al. | 2018 | 151.159 | -55.857 | â | â | â | 12.51 |
| Bica et al. | 2019 | 151.152 | -55.849 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 151.159 | -55.857 | 0.139 | -5.102 | 3.768 | â |
| Kharchenko et al. | 2016 | 151.145 | -55.854 | â | â | â | â |
| Kharchenko et al. | 2013 | 151.15 | -55.857 | â | -9.41 | 3.06 | â |
| Dias et al. | 2002 | 151.162 | -55.858 | â | -9.38 | -0.31 | 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 | 5.58 | 3.36 | â | 6 | â | 69 | â | â |
| Celli et al. | 2024 | â | â | â | 6 | â | 84 | â | â |
| Just et al. | 2023 | â | â | â | 6 | â | 54 | â | â |
| Cantat-Gaudin & Anders | 2020 | 5.95 | â | â | â | â | â | â | â |
| Soubiran et al. | 2018 | 5.95 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 5.95 | â | â | â | â | â | â | â |
| Kharchenko et al. | 2016 | 1.86 | 3.36 | â | 6 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.86 | 3.36 | â | 6 | â | â | â | â |
| Dias et al. | 2002 | 5.21 | 7.81 | â | 224 | â | â | â | â |
MOCA

