HSC 2304
0.11
UTI
0.74
CN
0.41
Cdens
0.75
CC3
0.06
Clit
0.27
Cdup
Nm (P>50%)
97
Core radius and density
1.7 [pc], 2.0 [pc-2]
- CN 0.74 Moderately populated
- Cdens 0.41 Loose
- CC3 0.75 High quality
- Clit 0.06 Rarely studied
- Cdup 0.27 Possibly duplicate
Overview
HSC 2304 is a moderately populated, loose object of high C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.
â ī¸ Warning: This is possibly a duplicate object, which shares a significant 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 | 147.326 | -60.149 | 0.903 | -7.072 | 4.131 | -0.464 |
| Yan et al. | 2026 | 147.315 | -60.184 | 0.899 | -7.092 | 4.119 | â |
| Hunt & Reffert | 2024 | 147.315 | -60.184 | 0.899 | -7.092 | 4.119 | -4.461 |
| Cavallo et al. | 2024 | 147.358 | -60.11 | 0.901 | â | â | â |
| Hunt & Reffert | 2023 | 147.315 | -60.184 | 0.899 | -7.092 | 4.119 | -4.461 |
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 | 1.06 | 0.2 | 0.39 | 187 | -0.070 | 182 | â | â |
| Yan et al. | 2026 | â | â | â | 186 | â | â | â | â |
| Hunt & Reffert | 2024 | 1.06 | 0.20 | 0.39 | 187 | â | 182(1) | â | â |
| Cavallo et al. | 2024 | 1.03 | 0.33 | â | 355 | -0.070 | â | â | â |
| Hunt & Reffert | 2023 | 1.06 | 0.20 | 0.39 | 187 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Yan et al. (2026)
Number of WDs: expected from single-star evolution N=6, with probability of formation through binary evolution >=0.5 N=0.
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as open cluster. CMD classes: 1.00 (50th percentile), true positive (human-assigned).
Hunt & Reffert (2023)
Classified as open cluster. CMD classes: 1.00 (50th percentile), true positive (human-assigned).