HSC 137
0.10
UTI
0.0
CN
0.14
Cdens
0.38
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad)
0.7 [N/pc2]
- CN 0.0 Sparse
- Cdens 0.14 Very loose
- CC3 0.38 Low quality
- Clit 0.0 Rarely studied
- Cdup 1.0 Unique
đĨ Members
đ Colab
đŦ Bayestar19
MOCA
đ CDS
đ Simbad
đ CDS (Îą, δ)
đ Simbad (Îą, δ)
MOCA
đ CDS
đ Simbad
đ CDS (Îą, δ)
đ Simbad (Îą, δ)
Overview
HSC 137 is a sparse, very loose object of low C3 quality. Its parallax locates it at a close distance, below the mid-plane, affected by low extinction. It is catalogued as a 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.
â ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) 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 | 282.055 | -24.464 | 1.887 | -3.059 | -8.003 | 9.875 |
| Hu & Soubiran | 2025 | 282.219 | -24.189 | â | â | â | â |
| Cavallo et al. | 2024 | 282.219 | -24.189 | 1.878 | â | â | â |
| Hunt & Reffert | 2023 | 281.57 | -24.35 | 1.873 | -3.044 | -8.029 | -2.234 |
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 | 0.51 | 0.89 | 0.71 | 410 | 0.035 | â | â | â |
| Hu & Soubiran | 2025 | â | â | â | â | -0.080(5) | â | â | â |
| Cavallo et al. | 2024 | 0.52 | 1.02 | â | 661 | 0.150 | â | â | â |
| Hunt & Reffert | 2023 | 0.50 | 0.76 | 0.71 | 159 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as a moving group.