FSR 0784
(Koposov 7)
0.24
UTI
0.0
CN
0.68
Cdens
0.75
CC3
0.0
Clit
0.84
Cdup
Stellar density (N50/rad)
3.4 [N/pc2]
- CN 0.0 Sparse
- Cdens 0.68 Moderately dense
- CC3 0.75 High quality
- Clit 0.0 Rarely studied
- Cdup 0.84 Very likely unique
Overview
FSR 0784 is a sparse, moderately dense object of high C3 quality. Its parallax locates it at a relatively close* distance, above the mid-plane, affected by extremely high extinction. It is catalogued as an intermediate-age cluster (see Parameters). It is rarely studied in the literature, with no articles listed in the last 16 years.
(*): The parallax distance estimate (~1.68 kpc) differs significantly from the median photometric distance (~4.76 kpc).
Note: This is very likely a unique object, which shares a small percentage of members with at least one previously reported entry, and a moderate percentage with at least one entry reported in the same catalogue. See table with shared members information.
â ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=0.84) 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 | 85.199 | 35.887 | 0.596 | 0.35 | -2.972 | -4.382 |
| Glushkova et al. | 2010 | 85.184 | 35.924 | â | â | â | â |
| Froebrich et al. | 2007 | 85.2 | 35.918 | â | â | â | 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 | 4.76 | 11.62 | â | 158 | â | â | â | â |
| Glushkova et al. | 2010 | 4.76 | 11.62 | â | 158 | â | â | â | â |
MOCA
