UBC 1614

Click to load Aladin Lite
0.46 UTI
0.29
CN
1.0
Cdens
0.38
CC3
0.31
Clit
1.0
Cdup
Radius (P>50% members) 2.6 [arcmin]
  • CN 0.29 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.38 Low quality
  • Clit 0.31 Poorly studied
  • Cdup 1.0 Unique

Overview

â„šī¸
UBC 1614 is a poorly populated, very dense object of low C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, old 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 a later reported entry. See table with shared members information.

Relatively close Low extinction Near-solar metallicity Old

Cavallo et al. (2024)
Gold sample.

Data

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 101.976 -7.13 0.409 -0.113 1.775 62.7
Hu & Soubiran 2025 101.964 -7.125 – – – –
Hunt & Reffert 2024 101.964 -7.123 0.411 -0.126 1.788 66.14
Cavallo et al. 2024 101.964 -7.125 0.411 – – –
Hunt & Reffert 2023 101.964 -7.123 0.411 -0.126 1.788 66.14
Castro-Ginard et al. 2022 101.98 -7.11 0.4 -0.12 1.77 62.37

💡 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] Bfr BSS
Hu & Soubiran 2025 – – – – -0.280* – – –
Hunt & Reffert 2024 – – – – – 269* – –
Cavallo et al. 2024 2.40 0.97 – 1175 0.170 – – –
Hunt & Reffert 2023 2.31 0.35 0.79 2254 – – – –
Castro-Ginard et al. 2022 2.79 0.85 – 470 – – – –

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 251 86.2 101.97 -7.13 0.41 -0.11 1.78 62.7 0.0

💡 Note: The % column shows the percentage of members that UBC 1614 shares with each listed object.

Visualization

â„šī¸