UBC 1466

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0.02 UTI
0.57
CN
1.0
Cdens
1.0
CC3
0.25
Clit
0.03
Cdup
Radius (P>50% members) 0.9 [arcmin]
  • CN 0.57 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.25 Poorly studied
  • Cdup 0.03 Very likely duplicate

Overview

â„šī¸
UBC 1466 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a very large distance, below the mid-plane, affected by high extinction. It is catalogued as a massive, metal-poor, intermediate-age cluster (see Parameters). It is poorly studied in the literature.

âš ī¸ Warning: This is very likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

Very distant High extinction Massive Metal-poor Intermediate age

Cavallo et al. (2024)
Gold sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 143.178 -53.273 0.091 -3.375 3.478 72.553
Hunt & Reffert 2024 143.178 -53.274 0.092 -3.369 3.472 72.562
Cavallo et al. 2024 143.194 -53.271 0.089 – – –
Hunt & Reffert 2023 143.178 -53.274 0.092 -3.369 3.472 72.562
Castro-Ginard et al. 2022 143.2 -53.28 0.09 -3.36 3.49 –

💡 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
Hunt & Reffert 2024 – – – – – 2430* – –
Cavallo et al. 2024 8.24 3.42 – 355 -0.500 – – –
Hunt & Reffert 2023 9.02 3.36 2.17 305 – – – –
Castro-Ginard et al. 2022 8.46 2.45 – 713 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
Kronberger 33 96.9 143.18 -53.27 0.09 -3.38 3.47 57.24 0.48

💡 Note: The % column shows the percentage of members that UBC 1466 shares with each listed object.

Visualization

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