OC 0697
0.13
UTI
0.77
CN
1.0
Cdens
1.0
CC3
0.25
Clit
0.2
Cdup
Stellar density (N50/rad)
25.1 [N/pc2]
- CN 0.77 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.25 Poorly studied
- Cdup 0.2 Likely duplicate
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 0697 is a rich, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a very massive, near-solar metallicity, very young cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It is poorly studied in the literature.
â ī¸ Warning: This is likely a duplicate object, which shares a large percentage of members with at least one previously 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 | 264.075 | -33.498 | 0.399 | -0.161 | -1.303 | -39.514 |
| Hunt & Reffert | 2024 | 264.06 | -33.493 | 0.397 | -0.177 | -1.293 | -27.856 |
| Cavallo et al. | 2024 | 264.074 | -33.487 | 0.397 | â | â | â |
| Hunt & Reffert | 2023 | 264.06 | -33.493 | 0.397 | -0.177 | -1.293 | -27.856 |
| Hao et al. | 2022 | 264.074 | -33.502 | 0.389 | -0.19 | -1.319 | -19.895 |
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 | 2.185 | 4.3 | 2.85 | 7 | 0.210 | 5455 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 5455(1) | â | â |
| Cavallo et al. | 2024 | 2.06 | 4.47 | â | 7 | -0.190 | â | â | â |
| Hunt & Reffert | 2023 | 2.31 | 4.30 | 2.85 | 7 | â | â | â | â |
| Hao et al. | 2022 | â | 3.86 | â | 2 | 0.611 | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
Palma et al. (2025)
Part of multiple system G51, along with UBC_565, Collinder_333, CWNU_2274 and UBC_566.
Cavallo et al. (2024)
Silver sample.