FSR 0384
(MWSC 3668)
0.76
UTI
0.61
CN
1.0
Cdens
0.75
CC3
0.71
Clit
1.0
Cdup
Nm (P>50%)
72
Core radius and density
1.2 [pc], 7.6 [pc-2]
- CN 0.61 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.71 Moderately studied
- Cdup 1.0 Unique
Overview
FSR 0384 is a moderately populated, very dense 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, but with a large variance across recent sources for the age and metallicity parameters (see Parameters). It is moderately studied in the literature.
Note: This object shares a moderate percentage of members with a later reported entry. 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 | 99999β | 342.912 | 56.101 | 0.492 | -3.506 | -1.741 | β |
| Li et al. | 2025 | 342.911 | 56.109 | 0.468 | -3.552 | -1.711 | β |
| Almeida et al. | 2025 | 342.915 | 56.112 | β | β | β | β |
| Zhang et al. | 2024 | 342.913 | 56.103 | β | β | β | β |
| Hunt & Reffert | 2024 | 342.913 | 56.103 | 0.497 | -3.499 | -1.766 | β |
| Cavallo et al. | 2024 | 342.931 | 56.122 | 0.497 | β | β | β |
| Hunt & Reffert | 2023 | 342.913 | 56.103 | 0.497 | -3.499 | -1.766 | β |
| Almeida et al. | 2023 | 342.914 | 56.109 | β | β | β | β |
| Just et al. | 2023 | 342.921 | 56.099 | β | β | β | β |
| Jadhav & Subramaniam | 2021 | 342.911 | 56.109 | β | β | β | β |
| Dias et al. | 2021 | 342.915 | 56.112 | 0.471 | -3.568 | -1.694 | β |
| Cantat-Gaudin et al. | 2020 | 342.911 | 56.109 | 0.468 | -3.552 | -1.711 | β |
| SΓ‘nchez et al. | 2020 | 342.917 | 56.109 | β | -4.041 | -1.506 | β |
| Zhong et al. | 2020 | 342.911 | 56.109 | β | -3.552 | -1.711 | -41.953 |
| Cantat-Gaudin & Anders | 2020 | 342.911 | 56.109 | 0.468 | -3.552 | -1.711 | β |
| Cantat-Gaudin et al. | 2018 | 342.911 | 56.109 | 0.468 | -3.552 | -1.711 | β |
| Dias et al. | 2018 | β | β | β | -1.99 | -1.76 | β |
| Sampedro et al. | 2017 | 342.917 | 56.109 | β | -1.53 | -4.19 | β |
| Kharchenko et al. | 2016 | 342.921 | 56.099 | β | β | β | β |
| Dias et al. | 2014 | 342.917 | 56.109 | β | -2.29 | -3.67 | β |
| Kharchenko et al. | 2013 | 342.927 | 56.103 | β | -0.67 | -0.38 | β |
| Kharchenko et al. | 2012 | 342.927 | 56.103 | β | -0.53 | -1.1 | β |
| Froebrich et al. | 2007 | 342.917 | 56.109 | β | β | β | β |
| Dias et al. | 2002 | 342.917 | 56.109 | β | -2.29 | -3.67 | β |
π‘ 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 | 99999β | 2.01 | 1.275 | 0.27 | 312 | 0.001 | 249 | 0.29 | 0 |
| Li et al. | 2025 | 1.68 | 1.08 | β | 555 | -0.173 | β | β | β |
| Almeida et al. | 2025 | 1.84 | 1.28 | β | 312 | β | 223 | β | β |
| Zhang et al. | 2024 | β | β | β | β | -0.160(1) | β | β | β |
| Hunt & Reffert | 2024 | 1.91 | 0.83 | 0.27 | 308 | β | 249(1) | β | β |
| Cavallo et al. | 2024 | 2.03 | 1.23 | β | 263 | 0.150 | β | β | β |
| Hunt & Reffert | 2023 | 1.91 | 0.83 | 0.27 | 308 | β | β | β | β |
| Almeida et al. | 2023 | 1.85 | 1.27 | β | 331 | 0.002 | 136(1) | 0.29 | β |
| Just et al. | 2023 | β | β | β | 7 | β | 358 | β | β |
| Jadhav & Subramaniam | 2021 | 1.92 | 1.01 | β | 427 | β | 301 | β | 0(1) |
| Dias et al. | 2021 | 1.84 | 1.28 | β | 312 | 0.003 | β | β | β |
| Cantat-Gaudin et al. | 2020 | 1.92 | 1.01 | β | 427 | β | β | β | β |
| Kounkel et al. | 2020 | 2.29 | 1.66 | β | 50 | β | β | β | β |
| Zhong et al. | 2020 | 2.01(1) | β | β | β | 0.000 | β | β | β |
| Cantat-Gaudin & Anders | 2020 | 2.01 | β | β | β | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 2.01 | β | β | β | β | β | β | β |
| Kharchenko et al. | 2016 | 3.40 | 2.37 | β | 7 | β | β | β | β |
| Kharchenko et al. | 2013 | 3.40 | 2.37 | β | 7 | β | β | β | β |
| Kharchenko et al. | 2012 | 4.80 | 1.91 | β | 841 | β | β | β | β |
| Dias et al. | 2002 | 4.80 | 1.91 | β | 841 | β | β | β | β |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Almeida et al. (2025)
Mass determination: intermediate fit. Isochrone match: good fit.
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).
Hu et al. (2021)
Ellipticities (core, all): e_core=0.1838, e_all=0.1552.