FSR 0366
(MWSC 3610)
0.17
UTI
0.0
CN
0.04
Cdens
0.5
CC3
0.16
Clit
1.0
Cdup
Nm (P>50%)
22
Core radius and density
2.1 [pc], 0.2 [pc-2]
- CN 0.0 Sparse
- Cdens 0.04 Very loose
- CC3 0.5 Intermediate quality
- Clit 0.16 Rarely studied
- Cdup 1.0 Unique
Overview
FSR 0366 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by high extinction. It is catalogued as a massive, metal-rich, young cluster, but with a large variance across recent sources for the age parameter (see Parameters). It is rarely studied in the literature.
Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.
â ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 334.556 | 59.059 | 0.249 | -3.427 | -2.442 | â |
| Hunt & Reffert | 2024 | 334.549 | 59.118 | 0.246 | -3.433 | -2.447 | â |
| Cavallo et al. | 2024 | 334.629 | 59.096 | 0.246 | â | â | â |
| Hunt & Reffert | 2023 | 334.549 | 59.118 | 0.246 | -3.433 | -2.447 | â |
| Bica et al. | 2019 | 334.66 | 59.017 | â | â | â | â |
| Sampedro et al. | 2017 | 334.663 | 59.014 | â | -2.73 | -2.59 | â |
| Froebrich et al. | 2007 | 334.663 | 59.014 | â | â | â | â |
| Dias et al. | 2002 | 334.663 | 59.014 | â | -1.82 | -1.33 | 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 | 3.82 | 3.35 | 2.57 | 26 | 0.510 | 1459 | â | â |
| Hunt & Reffert | 2024 | 3.82 | 3.35 | 2.57 | 6 | â | 1459(1) | â | â |
| Cavallo et al. | 2024 | 3.30 | 3.10 | â | 47 | 0.510 | â | â | â |
| Hunt & Reffert | 2023 | 3.82 | 3.35 | 2.57 | 6 | â | â | â | â |
| Dias et al. | 2002 | 5.61 | 3.48 | â | 519 | 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: 0.39 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.39 (50th percentile).