Gulliver 44
(FoF 2148)
0.90
UTI
0.77
CN
1.0
Cdens
0.75
CC3
1.0
Clit
1.0
Cdup
Radius (P>50% members)
9.2 [arcmin]
- CN 0.77 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
Gulliver 44 is a rich, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the age and metallicity parameters (see Parameters). It is very well-studied in the literature.
Relatively close
Moderate extinction
Near-solar metallicity
Intermediate age
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 127.25 | -38.09 | 0.806 | -0.642 | 2.35 | 14.636 |
| Li et al. | 2025 | 127.249 | -38.095 | 0.785 | -0.666 | 2.301 | â |
| Wei et al. | 2025 | 127.249 | -38.093 | 0.809 | -0.635 | 2.358 | â |
| Almeida et al. | 2025 | 127.231 | -38.099 | â | â | â | â |
| Hunt & Reffert | 2024 | 127.279 | -38.114 | 0.81 | -0.648 | 2.339 | 12.472 |
| Cavallo et al. | 2024 | 127.224 | -38.097 | 0.806 | â | â | â |
| Hunt & Reffert | 2023 | 127.279 | -38.114 | 0.81 | -0.648 | 2.339 | 12.472 |
| Almeida et al. | 2023 | 127.225 | -38.067 | â | â | â | â |
| He et al. | 2022 | 127.214 | -38.087 | 0.811 | -0.634 | 2.359 | â |
| Tarricq et al. | 2022 | 127.282 | -38.099 | 0.813 | -0.638 | 2.372 | â |
| Dias et al. | 2021 | 127.231 | -38.099 | 0.782 | -0.646 | 2.304 | 14.738 |
| Cantat-Gaudin et al. | 2020 | 127.249 | -38.095 | 0.785 | -0.666 | 2.301 | â |
| Cantat-Gaudin & Anders | 2020 | 127.249 | -38.095 | 0.785 | -0.666 | 2.301 | â |
| Liu & Pang | 2019 | 127.24 | -38.105 | 0.789 | -0.699 | 2.289 | â |
| Monteiro & Dias | 2019 | 127.249 | -38.095 | â | â | â | 2.21 |
| Bossini et al. | 2019 | 127.249 | -38.095 | â | â | â | â |
| Soubiran et al. | 2018 | 127.249 | -38.095 | â | â | â | 15.45 |
| Cantat-Gaudin et al. | 2018 | 127.249 | -38.095 | 0.785 | -0.666 | 2.301 | 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 |
|---|---|---|---|---|---|---|---|---|---|
| Li et al. | 2025 | 0.96 | 1.02 | â | 1804 | -0.258 | â | â | â |
| Wei et al. | 2025 | 1.78 | 1.28 | â | 576 | 0.500 | 605 | 0.72 | â |
| Almeida et al. | 2025 | 1.16 | 1.21 | â | 1016 | â | 455 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 572* | â | â |
| Cavallo et al. | 2024 | 1.27 | 1.65 | â | 324 | 0.250 | â | â | â |
| Hunt & Reffert | 2023 | 1.16 | 1.52 | 2.30 | 267 | â | â | â | â |
| Almeida et al. | 2023 | 1.18 | 1.47 | â | 614 | 0.031 | 379* | 0.72 | â |
| He et al. | 2022 | â | 1.75 | â | 355 | â | â | â | â |
| Tarricq et al. | 2022 | 1.19 | â | â | 550 | â | â | â | â |
| Dias et al. | 2021 | 1.16 | 1.21 | â | 1016 | 0.102 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 1.22 | 0.78 | â | 447 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 1.23 | â | â | â | â | â | â | â |
| Liu & Pang | 2019 | â | â | â | 562 | 0.500 | â | â | â |
| Monteiro & Dias | 2019 | 1.21 | 1.21 | â | 735 | 0.051 | â | â | â |
| Bossini et al. | 2019 | 0.97 | 0.50 | â | 1521 | 0.000 | â | â | â |
| Soubiran et al. | 2018 | 1.23 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 1.23 | â | â | â | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Almeida et al. (2025)
Mass determination: good fit. Isochrone match: good fit.
Cavallo et al. (2024)
Gold sample.