OC 0497
0.48
UTI
0.26
CN
1.0
Cdens
1.0
CC3
0.06
Clit
1.0
Cdup
Nm (P>50%)
26
Core radius and density
0.5 [pc], 15 [pc-2]
- CN 0.26 Poorly populated
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.06 Rarely studied
- Cdup 1.0 Unique
Overview
OC 0497 is a poorly populated, very dense object of very high C3 quality. Its parallax locates it at a close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It is rarely studied in the literature.
Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 137.854 | -45.584 | 1.321 | -8.431 | 3.923 | -1.189 |
| Hunt & Reffert | 2024 | 137.852 | -45.568 | 1.291 | -8.559 | 4.068 | -2.182 |
| Cavallo et al. | 2024 | 137.885 | -45.547 | 1.313 | â | â | â |
| Hunt & Reffert | 2023 | 137.852 | -45.568 | 1.291 | -8.559 | 4.068 | -2.182 |
| Hao et al. | 2022 | 137.852 | -45.573 | 1.328 | -8.436 | 3.893 | â |
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 | 0.73 | 1.53 | 2.06 | 3 | 0.128 | 89 | â | â |
| Hunt & Reffert | 2024 | 0.73 | 1.53 | 2.06 | 4 | â | 89(1) | â | â |
| Cavallo et al. | 2024 | 1.01 | 1.78 | â | 2 | 0.040 | â | â | â |
| Hunt & Reffert | 2023 | 0.73 | 1.53 | 2.06 | 4 | â | â | â | â |
| Hao et al. | 2022 | â | 0.86 | â | 2 | 0.216 | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Cavallo et al. (2024)
Bronze sample.
Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.73 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.73 (50th percentile).