FSR 0596
0.42
UTI
0.52
CN
0.31
Cdens
0.75
CC3
0.26
Clit
1.0
Cdup
Nm (P>50%)
55
Core radius and density
1.5 [pc], 1.6 [pc-2]
- CN 0.52 Moderately populated
- Cdens 0.31 Loose
- CC3 0.75 High quality
- Clit 0.26 Poorly studied
- Cdup 1.0 Unique
Overview
FSR 0596 is a moderately populated, loose object of high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is poorly studied in the literature.
Note: This object shares a significant percentage of members with 5 later reported entries. See table with shared members information.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 37.477 | 58.126 | 0.404 | -0.476 | -0.913 | -51.173 |
| Hunt & Reffert | 2024 | 37.483 | 58.123 | 0.4 | -0.492 | -0.907 | â |
| Cavallo et al. | 2024 | 37.478 | 58.12 | 0.4 | â | â | â |
| Hunt & Reffert | 2023 | 37.483 | 58.123 | 0.4 | -0.492 | -0.907 | â |
| Bica et al. | 2019 | 37.467 | 58.11 | â | â | â | â |
| Dib et al. | 2018 | 37.432 | 58.1 | â | â | â | â |
| Sampedro et al. | 2017 | 37.467 | 58.11 | â | â | â | â |
| Joshi et al. | 2016 | 37.432 | 58.1 | â | â | â | â |
| Dias et al. | 2014 | 37.467 | 58.11 | â | -0.65 | -1.82 | â |
| Froebrich et al. | 2007 | 37.467 | 58.11 | â | â | â | â |
| Dias et al. | 2002 | 37.467 | 58.11 | â | -1.49 | 2.97 | 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 | 1.905 | 1.99 | 0.46 | 740 | -0.070 | 273 | â | â |
| Hunt & Reffert | 2024 | 2.39 | 1.99 | 0.46 | 26 | â | 273(1) | â | â |
| Cavallo et al. | 2024 | 2.61 | 2.14 | â | 66 | -0.070 | â | â | â |
| Hunt & Reffert | 2023 | 2.39 | 1.99 | 0.46 | 26 | â | â | â | â |
| Dib et al. | 2018 | 1.42 | â | â | 1413 | â | â | â | â |
| Joshi et al. | 2016 | 1.42 | 1.64 | â | 1413 | â | â | â | â |
| Dias et al. | 2002 | 1.42 | 1.64 | â | 1413 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as open cluster. CMD class: 1.00 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 1.00 (50th percentile).