HSC 297
0.12
UTI
0.0
CN
0.21
Cdens
0.5
CC3
0.0
Clit
0.84
Cdup
Radius (P>50% members)
30.2 [arcmin]
- CN 0.0 Sparse
- Cdens 0.21 Very loose
- CC3 0.5 Intermediate quality
- Clit 0.0 Rarely studied
- Cdup 0.84 Very likely unique
Overview
HSC 297 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a close distance, above the mid-plane, affected by low extinction. It is catalogued as a young cluster (see Parameters). It was recently reported in the literature.
Note: This is very likely a unique object, which shares a 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=0.84) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.
Very close
Low extinction
Young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 270.704 | 2.757 | 1.942 | 0.417 | -8.662 | -4.844 |
| Hunt & Reffert | 2023 | 270.786 | 2.736 | 2.206 | 0.382 | -8.628 | -24.242 |
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] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| Hunt & Reffert | 2023 | 0.44 | 0.22 | 0.53 | 29 | â | â | â | â |
Hunt & Reffert (2024)
Classified as a moving group.