FSR 0952
(MWSC 775)
0.23
UTI
0.29
CN
0.05
Cdens
0.5
CC3
0.16
Clit
1.0
Cdup
Nm (P>50%)
29
Core radius and density
3.3 [pc], 0.3 [pc-2]
- CN 0.29 Poorly populated
- Cdens 0.05 Very loose
- CC3 0.5 Intermediate quality
- Clit 0.16 Rarely studied
- Cdup 1.0 Unique
Overview
FSR 0952 is a poorly populated, very loose object of intermediate C3 quality. Its parallax locates it at a moderate* distance, below the mid-plane, affected by moderate extinction. It is catalogued as an old cluster (see Parameters). It is rarely studied in the literature.
(*): The parallax distance estimate (~4.20 kpc) differs significantly from the median photometric distance (~1.99 kpc).
Note: This object shares a large percentage of members with 2 later reported entries. 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 | 92.547 | 13.053 | 0.238 | -0.525 | -0.633 | â |
| Just et al. | 2023 | 92.564 | 13.018 | â | â | â | â |
| Dib et al. | 2018 | 92.572 | 13.017 | â | â | â | â |
| Sampedro et al. | 2017 | 92.562 | 13.013 | â | -1.25 | -3.06 | â |
| Kharchenko et al. | 2016 | 92.564 | 13.018 | â | â | â | â |
| Kharchenko et al. | 2013 | 92.572 | 13.017 | â | -1.16 | -1.84 | â |
| Froebrich et al. | 2007 | 92.562 | 13.013 | â | â | â | â |
| Dias et al. | 2002 | 92.562 | 13.013 | â | -2.79 | -1.23 | 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 | 1.99 | 1.97 | â | 1274 | â | 213 | â | â |
| Just et al. | 2023 | â | â | â | 1274 | â | 213 | â | â |
| Dib et al. | 2018 | 1.99 | â | â | 1274 | â | â | â | â |
| Kharchenko et al. | 2016 | 1.99 | 1.97 | â | 1274 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.99 | 1.97 | â | 1274 | â | â | â | â |
| Dias et al. | 2002 | 1.99 | 1.97 | â | 1274 | â | â | â | â |
MOCA
