FSR 0059
(MWSC 2923)
0.23
UTI
0.0
CN
0.12
Cdens
0.38
CC3
0.32
Clit
1.0
Cdup
Nm (P>50%)
16
Core radius and density
2.1 [pc], 0.6 [pc-2]
- CN 0.0 Sparse
- Cdens 0.12 Very loose
- CC3 0.38 Low quality
- Clit 0.32 Poorly studied
- Cdup 1.0 Unique
Overview
FSR 0059 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate* distance, near the mid-plane, affected by high extinction. It is catalogued as an intermediate-age cluster (see Parameters). It is poorly studied in the literature.
(*): The parallax distance estimate (~3.42 kpc) differs significantly from the median photometric distance (~1.55 kpc).
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 | 277.204 | -11.964 | 0.292 | -1.757 | -3.289 | â |
| Just et al. | 2023 | 277.258 | -11.969 | â | â | â | â |
| Bica et al. | 2019 | 277.265 | -11.979 | â | â | â | â |
| Dias et al. | 2018 | â | â | â | -0.01 | -3.69 | â |
| Dib et al. | 2018 | 277.266 | -11.967 | â | â | â | â |
| Sampedro et al. | 2017 | 277.267 | -11.975 | â | -2.32 | 1.24 | â |
| Joshi et al. | 2016 | 277.266 | -11.967 | â | â | â | â |
| Kharchenko et al. | 2016 | 277.258 | -11.969 | â | â | â | â |
| Dias et al. | 2014 | 277.267 | -11.975 | â | 0.36 | -1.25 | â |
| Kharchenko et al. | 2013 | 277.266 | -11.967 | â | -2.41 | -3.61 | â |
| Morales et al. | 2013 | 277.267 | -11.975 | â | â | â | â |
| Froebrich et al. | 2007 | 277.267 | -11.975 | â | â | â | â |
| Dias et al. | 2002 | 277.267 | -11.975 | â | 0.36 | -1.25 | 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 | 1.55 | 3.42 | â | 251 | â | 112 | â | â |
| Just et al. | 2023 | â | â | â | 251 | â | 112 | â | â |
| Dib et al. | 2018 | 1.55 | â | â | 251 | â | â | â | â |
| Joshi et al. | 2016 | 1.55 | 3.42 | â | 251 | â | â | â | â |
| Kharchenko et al. | 2016 | 1.55 | 3.42 | â | 251 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.55 | 3.42 | â | 251 | â | â | â | â |
| Dias et al. | 2002 | 1.55 | 3.42 | â | 251 | â | â | â | â |
MOCA

Morales et al. (2013)
Classified as morphological type 'OC2' (totally exposed cluster without correlation with ATLASGAL emission). Morphological flag: exposed cluster, without submm emission.