OC 0602
0.50
UTI
0.33
CN
0.67
Cdens
1.0
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad)
3.3 [N/pc2]
- CN 0.33 Poorly populated
- Cdens 0.67 Moderately dense
- CC3 1.0 Very high quality
- Clit 0.25 Poorly 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
OC 0602 is a poorly populated, moderately dense object of very high C3 quality. Its parallax locates it at a relatively close distance, above 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 metallicity parameter (see Parameters). It is poorly studied in the literature.
Note: This object shares a large percentage of members with 2 later reported entries. 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 | 205.324 | -56.671 | 0.584 | -4.455 | -1.278 | -15.574 |
| Hunt & Reffert | 2024 | 205.306 | -56.651 | 0.589 | -4.455 | -1.283 | -16.702 |
| Cavallo et al. | 2024 | 205.408 | -56.688 | 0.589 | â | â | â |
| Hunt & Reffert | 2023 | 205.306 | -56.651 | 0.589 | -4.455 | -1.283 | -16.702 |
| Hao et al. | 2022 | 205.293 | -56.642 | 0.59 | -4.473 | -1.311 | -15.026 |
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 | 1.535 | 0.88 | 0.39 | 398 | 0.266 | 126 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 126(1) | â | â |
| Cavallo et al. | 2024 | 1.47 | 0.88 | â | 398 | -0.080 | â | â | â |
| Hunt & Reffert | 2023 | 1.60 | 0.66 | 0.39 | 438 | â | â | â | â |
| Hao et al. | 2022 | â | 0.98 | â | 398 | 0.611 | 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.