HSC 1449
0.20
UTI
0.0
CN
0.14
Cdens
0.38
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members)
12.2 [arcmin]
- CN 0.0 Sparse
- Cdens 0.14 Very loose
- CC3 0.38 Low quality
- Clit 0.25 Poorly studied
- Cdup 1.0 Unique
Overview
HSC 1449 is a sparse, very loose object of low C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It was recently reported in the literature.
Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.
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.
Relatively close
Moderate extinction
Near-solar metallicity
Intermediate age
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 79.894 | 20.634 | 0.625 | 0.289 | -3.96 | 22.218 |
| Zhang et al. | 2024 | 79.905 | 20.62 | â | â | â | â |
| Hunt & Reffert | 2024 | 79.905 | 20.62 | 0.626 | 0.304 | -3.961 | 22.213 |
| Cavallo et al. | 2024 | 79.825 | 20.64 | 0.633 | â | â | â |
| Hunt & Reffert | 2023 | 79.905 | 20.62 | 0.626 | 0.304 | -3.961 | 22.213 |
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 |
|---|---|---|---|---|---|---|---|---|---|
| Zhang et al. | 2024 | â | â | â | â | -0.393* | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 109* | â | â |
| Cavallo et al. | 2024 | 1.69 | 0.97 | â | 372 | 0.620 | â | â | â |
| Hunt & Reffert | 2023 | 1.47 | 1.49 | 1.31 | 177 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Gold sample.