FSR 1032
(MWSC 926)
0.64
UTI
0.51
CN
1.0
Cdens
1.0
CC3
0.35
Clit
1.0
Cdup
Nm (P>50%)
52
Core radius and density
1.2 [pc], 6.6 [pc-2]
- CN 0.51 Moderately populated
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.35 Poorly studied
- Cdup 1.0 Unique
Overview
FSR 1032 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is poorly studied in the literature.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 99.069 | 4.011 | 0.401 | -1.152 | -3.152 | 44.491 |
| Hunt & Reffert | 2024 | 99.072 | 4.011 | 0.427 | -1.122 | -3.115 | 38.088 |
| Hunt & Reffert | 2023 | 99.072 | 4.011 | 0.427 | -1.122 | -3.115 | 38.088 |
| Just et al. | 2023 | 99.06 | 4.002 | â | â | â | â |
| Cantat-Gaudin et al. | 2020 | 99.072 | 4.011 | 0.456 | -1.372 | -3.174 | â |
| Zhong et al. | 2020 | 99.072 | 4.011 | â | -1.372 | -3.174 | 22.275 |
| Cantat-Gaudin & Anders | 2020 | 99.072 | 4.011 | 0.456 | -1.372 | -3.174 | â |
| Soubiran et al. | 2018 | 99.072 | 4.011 | â | â | â | 51.96 |
| Bica et al. | 2019 | 99.073 | 4.016 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 99.072 | 4.011 | 0.456 | -1.372 | -3.174 | â |
| Kharchenko et al. | 2016 | 99.06 | 4.002 | â | â | â | â |
| Kharchenko et al. | 2013 | 99.067 | 4.0 | â | -1.9 | -0.37 | â |
| Froebrich et al. | 2007 | 99.067 | 4.012 | â | â | â | 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 | 2.06 | 4.67 | 1.08 | 525 | 0.000 | 258 | â | â |
| Hunt & Reffert | 2024 | 2.11 | 4.67 | 1.08 | 604 | â | 418(1) | â | â |
| Hunt & Reffert | 2023 | 2.11 | 4.67 | 1.08 | 604 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 525 | â | 98 | â | â |
| Kounkel et al. | 2020 | 2.73 | 4.39 | â | 16 | â | â | â | â |
| Zhong et al. | 2020 | 2.06(1) | â | â | â | 0.000 | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 2.06 | â | â | â | â | â | â | â |
| Soubiran et al. | 2018 | 2.06 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 2.06 | â | â | â | â | â | â | â |
| Kharchenko et al. | 2016 | 1.94 | 5.45 | â | 525 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.94 | 5.45 | â | 525 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.94 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.94 (50th percentile).