UBC 288
0.20
UTI
0.83
CN
1.0
Cdens
1.0
CC3
0.03
Clit
0.35
Cdup
Nm (P>50%)
319
Core radius and density
1.4 [pc], 9.6 [pc-2]
- CN 0.83 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.03 Rarely studied
- Cdup 0.35 Possibly 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
UBC 288 is a rich, very dense object of very high C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is rarely studied in the literature.
â ī¸ Warning: This is possibly a duplicate object, which shares a significant percentage of members with at least one previously reported entry. See table with shared members information.
Note: This object contains blue stragglers according to at least one source.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 191.007 | -58.095 | 0.527 | -2.212 | -1.257 | -8.79 |
| Li et al. | 2023 | 191.0 | -58.083 | 0.52 | -2.21 | -1.26 | â |
| Castro-Ginard et al. | 2020 | 190.972 | -58.097 | 0.505 | -2.184 | -1.277 | 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 | 2.125 | 1.62 | â | 740 | -0.006 | â | â | 1 |
| Li et al. | 2023 | 2.40 | 1.15 | â | 1000 | -0.006 | â | â | 1(1) |
| Kounkel et al. | 2020 | 1.85 | 2.09 | â | 479 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
Castro-Ginard et al. (2020)
Coincidence with Sim et al. (2019, J. Korean Astron. Soc., 52, 145) or Liu & Pang (2019ApJS..245...32L), see Sect. 4.1.5.