HSC 1504
0.07
UTI
0.0
CN
0.17
Cdens
0.5
CC3
0.25
Clit
0.28
Cdup
Stellar density (N50/rad)
0.8 [N/pc2]
- CN 0.0 Sparse
- Cdens 0.17 Very loose
- CC3 0.5 Intermediate quality
- Clit 0.25 Poorly studied
- Cdup 0.28 Possibly duplicate
Overview
HSC 1504 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a moderate distance, above 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 metallicity parameter (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 | 93.576 | 21.116 | 0.496 | 0.157 | -2.195 | 35.586 |
| Zhang et al. | 2024 | 93.57 | 21.096 | â | â | â | â |
| Hunt & Reffert | 2024 | 93.57 | 21.096 | 0.498 | 0.152 | -2.19 | 35.56 |
| Cavallo et al. | 2024 | 93.62 | 21.117 | 0.499 | â | â | â |
| Hunt & Reffert | 2023 | 93.57 | 21.096 | 0.498 | 0.152 | -2.19 | 35.56 |
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 | 2.13 | 1.675 | 1.34 | 22 | 0.194 | 204 | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.223(1) | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 204(1) | â | â |
| Cavallo et al. | 2024 | 2.41 | 1.90 | â | 19 | 0.610 | â | â | â |
| Hunt & Reffert | 2023 | 1.85 | 1.45 | 1.34 | 26 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Palma et al. (2025)
Part of multiple system G118, along with NGC_2175, Pismis_27, UBC_1303 and FSR_0902.
Cavallo et al. (2024)
Gold sample.