HSC 2695
0.05
UTI
0.0
CN
0.07
Cdens
0.38
CC3
0.0
Clit
0.56
Cdup
Stellar density (N50/rad)
0.4 [N/pc2]
- CN 0.0 Sparse
- Cdens 0.07 Very loose
- CC3 0.38 Low quality
- Clit 0.0 Rarely studied
- Cdup 0.56 Likely 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 2695 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by very high extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It was recently reported in the literature.
Note: This is likely a unique object, which shares a moderate 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=0.56) 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 | 230.221 | -57.308 | 0.28 | -2.417 | -2.143 | -38.407 |
| Cavallo et al. | 2024 | 230.276 | -57.276 | 0.293 | â | â | â |
| Hunt & Reffert | 2023 | 230.355 | -57.416 | 0.296 | -2.43 | -2.119 | -38.784 |
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 | 3.385 | 5.355 | 2.4 | 31 | 0.170 | â | â | â |
| Cavallo et al. | 2024 | 3.66 | 5.04 | â | 24 | 0.170 | â | â | â |
| Hunt & Reffert | 2023 | 3.11 | 5.67 | 2.40 | 38 | â | â | â | â |
Cavallo et al. (2024)
Wood sample.
Hunt & Reffert (2024)
Classified as a moving group.