UBC 481
0.18
UTI
0.75
CN
0.75
Cdens
0.75
CC3
0.25
Clit
0.32
Cdup
Stellar density (N50/rad)
3.7 [N/pc2]
- CN 0.75 Rich
- Cdens 0.75 Dense
- CC3 0.75 High quality
- Clit 0.25 Poorly studied
- Cdup 0.32 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 481 is a rich, dense object of high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is poorly 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.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 130.881 | -45.808 | 0.657 | -5.028 | 4.643 | 13.238 |
| Hunt & Reffert | 2024 | 130.886 | -45.852 | 0.657 | -5.021 | 4.646 | 20.351 |
| Cavallo et al. | 2024 | 130.901 | -45.784 | 0.658 | â | â | â |
| Hunt & Reffert | 2023 | 130.886 | -45.852 | 0.657 | -5.021 | 4.646 | 20.351 |
| Castro-Ginard et al. | 2020 | 130.845 | -45.771 | 0.65 | -5.066 | 4.642 | 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 | 1.47 | 1.3 | 2.21 | 34 | -0.020 | 505 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 505(1) | â | â |
| Cavallo et al. | 2024 | 1.50 | 1.37 | â | 20 | -0.020 | â | â | â |
| Hunt & Reffert | 2023 | 1.44 | 1.23 | 2.21 | 48 | â | 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.
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.