FSR 0846
(MWSC 674)
0.15
UTI
0.0
CN
0.04
Cdens
0.25
CC3
0.23
Clit
1.0
Cdup
Nm (P>50%)
16
Core radius and density
2.2 [pc], 0.2 [pc-2]
- CN 0.0 Sparse
- Cdens 0.04 Very loose
- CC3 0.25 Low quality
- Clit 0.23 Rarely studied
- Cdup 1.0 Unique
Overview
FSR 0846 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 a young cluster (see Parameters). It is rarely studied in the literature.
(*): The parallax distance estimate (~3.47 kpc) differs significantly from the median photometric distance (~1.88 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 | 87.211 | 26.362 | 0.288 | -0.258 | -1.859 | 40.28 |
| Just et al. | 2023 | 87.201 | 26.366 | â | â | â | â |
| Dib et al. | 2018 | 87.21 | 26.365 | â | â | â | â |
| Loktin & Popova | 2017 | 87.18 | 26.368 | â | 0.168 | -1.671 | â |
| Sampedro et al. | 2017 | 87.183 | 26.368 | â | 0.5 | 0.33 | â |
| Kharchenko et al. | 2016 | 87.201 | 26.366 | â | â | â | â |
| Kharchenko et al. | 2013 | 87.21 | 26.365 | â | 0.17 | -4.59 | â |
| Camargo et al. | 2012 | 87.183 | 26.368 | â | â | â | â |
| Froebrich et al. | 2007 | 87.183 | 26.368 | â | â | â | â |
| Dias et al. | 2002 | 87.183 | 26.368 | â | 1.99 | -0.15 | 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 | 1.88 | 3.22 | â | 20 | â | 71 | â | â |
| Just et al. | 2023 | â | â | â | 20 | â | 71 | â | â |
| Dib et al. | 2018 | 1.88 | â | â | 20 | â | â | â | â |
| Loktin & Popova | 2017 | 1.50 | 0.60 | â | 16 | â | â | â | â |
| Kharchenko et al. | 2016 | 1.88 | 3.22 | â | 20 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.88 | 3.22 | â | 20 | â | â | â | â |
| Camargo et al. | 2012 | 2.48 | 2.98 | â | 3 | â | â | â | â |
| Dias et al. | 2002 | 1.88 | 3.22 | â | 20 | â | â | â | â |
MOCA
