Gulliver 16
0.46
UTI
0.75
CN
1.0
Cdens
0.75
CC3
0.25
Clit
0.77
Cdup
Radius (P>50% members)
2.5 [arcmin]
- CN 0.75 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.25 Poorly studied
- Cdup 0.77 Very likely unique
Overview
Gulliver 16 is a rich, very dense object of high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the age parameter (see Parameters). It is poorly studied in the literature, with no articles listed in the last 6 years.
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.
Distant
Moderate extinction
Near-solar metallicity
Young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 23.423 | 60.749 | 0.215 | -1.28 | -0.654 | -37.022 |
| Cantat-Gaudin et al. | 2020 | 23.433 | 60.751 | 0.208 | -1.249 | -0.614 | â |
| Cantat-Gaudin & Anders | 2020 | 23.433 | 60.751 | 0.208 | -1.249 | -0.614 | â |
| Monteiro & Dias | 2019 | 23.433 | 60.751 | â | â | â | 3.016 |
| Cantat-Gaudin et al. | 2018 | 23.433 | 60.751 | 0.208 | -1.249 | -0.614 | 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 |
|---|---|---|---|---|---|---|---|---|---|
| Cantat-Gaudin et al. | 2020 | 4.90 | 1.39 | â | 141 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 4.22 | â | â | â | â | â | â | â |
| Monteiro & Dias | 2019 | 8.76 | 1.81 | â | 7 | 0.050 | â | â | â |
| Cantat-Gaudin et al. | 2018 | 4.22 | â | â | â | â | â | â | â |

