HSC 1629
0.08
UTI
0.37
CN
1.0
Cdens
0.25
CC3
0.25
Clit
0.19
Cdup
Stellar density (N50/rad)
6.5 [N/pc2]
- CN 0.37 Poorly populated
- Cdens 1.0 Very dense
- CC3 0.25 Low quality
- Clit 0.25 Poorly studied
- Cdup 0.19 Likely duplicate
Overview
HSC 1629 is a poorly populated, very dense object of low C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It was recently reported in the literature.
â ī¸ Warning: This is likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 98.999 | 5.506 | 0.645 | -1.217 | 0.564 | 71.11 |
| Liu et al. | 2025 | 99.02 | 5.51 | 0.65 | -1.21 | 0.58 | 71.12 |
| Hunt & Reffert | 2024 | 99.019 | 5.515 | 0.65 | -1.205 | 0.583 | 71.121 |
| Cavallo et al. | 2024 | 98.936 | 5.456 | 0.65 | â | â | â |
| Hunt & Reffert | 2023 | 99.019 | 5.515 | 0.65 | -1.205 | 0.583 | 71.121 |
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] | Bfrac | BSS |
|---|---|---|---|---|---|---|---|---|---|
| UCC | 99999â | 1.46 | 0.68 | 1.08 | 21 | 0.140 | 146 | â | â |
| Liu et al. | 2025 | 2.14 | 0.33 | â | 17 | â | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 146(1) | â | â |
| Cavallo et al. | 2024 | 1.46 | 1.06 | â | 21 | 0.140 | â | â | â |
| Hunt & Reffert | 2023 | 1.41 | 0.68 | 1.08 | 29 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Liu et al. (2025)
Classified as primordial binary cluster 124 along with Collinder_106, and as primordial binary cluster 125 along with Collinder_107, and as primordial binary cluster 281 along with NGC_2244, and of multiple system 42 along with NGC_2244, Collinder_106 and Collinder_107.
Palma et al. (2025)
Part of multiple system G20, along with Desvoivres_2, NGC_2244, Collinder_107 and Collinder_106.
Cavallo et al. (2024)
Gold sample.