Gulliver 29
0.74
UTI
0.82
CN
1.0
Cdens
1.0
CC3
0.44
Clit
1.0
Cdup
Radius (P>50% members)
19.3 [arcmin]
- CN 0.82 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.44 Poorly studied
- Cdup 1.0 Unique
Overview
Gulliver 29 is a rich, very dense object of very high C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a massive, near-solar metallicity, very young cluster (see Parameters). It is poorly studied in the literature.
Note: This object shares a moderate percentage of members with 3 later reported entries. See table with shared members information.
Relatively close
Moderate extinction
Massive
Near-solar metallicity
Very young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 256.671 | -35.259 | 0.903 | 1.279 | -2.204 | 5.004 |
| Celli et al. | 2024 | 256.745 | -35.205 | â | â | â | â |
| He et al. | 2022 | 256.744 | -35.478 | 0.903 | 1.261 | -2.274 | â |
| Cantat-Gaudin et al. | 2020 | 256.745 | -35.205 | 0.905 | 1.325 | -2.206 | â |
| Cantat-Gaudin & Anders | 2020 | 256.745 | -35.205 | 0.905 | 1.325 | -2.206 | â |
| Monteiro & Dias | 2019 | 256.745 | -35.205 | â | â | â | 2.144 |
| Soubiran et al. | 2018 | 256.745 | -35.205 | â | â | â | 3.46 |
| Cantat-Gaudin et al. | 2018 | 256.745 | -35.205 | 0.905 | 1.325 | -2.206 | 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 |
|---|---|---|---|---|---|---|---|---|---|
| Celli et al. | 2024 | â | â | â | 11 | â | 1591 | â | â |
| He et al. | 2022 | â | 2.00 | â | 9 | â | â | â | â |
| Cantat-Gaudin et al. | 2020 | 1.18 | 1.02 | â | 11 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 1.07 | â | â | â | â | â | â | â |
| Monteiro & Dias | 2019 | 0.95 | 2.20 | â | 16 | 0.006 | â | â | â |
| Soubiran et al. | 2018 | 1.07 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 1.07 | â | â | â | â | â | â | â |

