FSR 1712
(MWSC 2332; GLIMPSE 68; Mercer 68)
- 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
(*): 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.
⚠️ 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.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | – | 238.711 | -52.478 | 0.549 | -5.654 | -5.486 | – |
| Just et al. | 2023 | 238.668 | -52.479 | – | – | – | – |
| Bica et al. | 2019 | 238.694 | -52.528 | – | – | – | – |
| Kharchenko et al. | 2016 | 238.668 | -52.479 | – | – | – | – |
| Kharchenko et al. | 2013 | 238.68 | -52.48 | – | -4.57 | -2.67 | – |
| Froebrich et al. | 2007 | 238.692 | -52.502 | – | – | – | – |
💡 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 | – | – | – | 398 | – | 76 | – | – |
| Kharchenko et al. | 2016 | 1.14 | 2.13 | – | 398 | – | – | – | – |
| Kharchenko et al. | 2013 | 1.14 | 2.13 | – | 398 | – | – | – | – |
💡 Note: The parameters are sometimes transformed from their original values to match the format of the columns shown here, see FAQ. The columns DAv, Bfr, BSS correspond to differential extinction, binary fraction, and blue stragglers, respectively. BSS values can be listed as fractions or integers.
