HSC 675
0.05
UTI
0.0
CN
0.01
Cdens
0.25
CC3
0.0
Clit
0.96
Cdup
Stellar density (N50/rad)
0.1 [N/pc2]
- CN 0.0 Sparse
- Cdens 0.01 Very loose
- CC3 0.25 Low quality
- Clit 0.0 Rarely studied
- Cdup 0.96 Unique
Overview
HSC 675 is a sparse, very loose object of low C3 quality. Its parallax locates it at a large distance, below the mid-plane, affected by moderate extinction. It is catalogued as a massive, near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the age parameter (see Parameters). It was recently reported in the literature.
Note: This is a unique object, which shares a very small percentage of members with at least one previously reported entry. See table with shared members information.
â ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=0.96) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 315.722 | 44.768 | 0.105 | -2.602 | -3.329 | -86.789 |
| Hunt & Reffert | 2024 | 315.711 | 44.764 | 0.107 | -2.596 | -3.344 | -86.906 |
| Cavallo et al. | 2024 | 315.743 | 44.753 | 0.107 | â | â | â |
| Hunt & Reffert | 2023 | 315.711 | 44.764 | 0.107 | -2.596 | -3.344 | -86.906 |
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 | 7.725 | 2.54 | 2.19 | 458 | -0.020 | 1221 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 1221(1) | â | â |
| Cavallo et al. | 2024 | 7.14 | 1.46 | â | 813 | -0.020 | â | â | â |
| Hunt & Reffert | 2023 | 8.31 | 3.62 | 2.19 | 104 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Cavallo et al. (2024)
Wood sample.