FSR 1712
(MWSC 2332; GLIMPSE 68; Mercer 68)
0.15
UTI
0.0
CN
0.25
Cdens
0.12
CC3
0.31
Clit
0.76
Cdup
Radius (P>50% members)
7.9 [arcmin]
- CN 0.0 Sparse
- Cdens 0.25 Loose
- CC3 0.12 Very low quality
- Clit 0.31 Poorly studied
- Cdup 0.76 Very likely unique
Overview
FSR 1712 is a sparse, loose object of very low C3 quality. Its parallax locates it at a relatively close* distance, near the mid-plane, affected by moderate extinction. It is catalogued as an intermediate-age cluster (see Parameters). It is poorly studied in the literature.
(*): The parallax distance estimate (~1.82 kpc) differs significantly from the median photometric distance (~1.14 kpc).
Note: This is very likely a unique object, which shares a small percentage of members with at least one previously reported entry. See table with shared members information.
â ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=0.76) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.
Relatively close
Moderate extinction
Intermediate age
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 238.711 | -52.478 | 0.549 | -5.654 | -5.486 | â |
| Just et al. | 2023 | 238.668 | -52.479 | â | â | â | â |
| Bica et al. | 2019 | 238.694 | -52.528 | â | â | â | â |
| Kharchenko et al. | 2016 | 238.668 | -52.479 | â | â | â | â |
| Kharchenko et al. | 2013 | 238.68 | -52.48 | â | -4.57 | -2.67 | â |
| Froebrich et al. | 2007 | 238.692 | -52.502 | 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] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| Just et al. | 2023 | â | â | â | 398 | â | 76 | â | â |
| Kharchenko et al. | 2016 | 1.14 | 2.13 | â | 398 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.14 | 2.13 | â | 398 | â | â | â | â |
