UBC 1447

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0.43 UTI
0.25
CN
1.0
Cdens
0.38
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 2.8 [arcmin]
  • CN 0.25 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.38 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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UBC 1447 is a poorly populated, very dense object of low C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, very young cluster (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 High extinction Near-solar metallicity Very young

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 – 133.34 -46.035 0.481 -5.677 4.378 –
Hunt & Reffert 2024 133.342 -46.039 0.484 -5.672 4.398 –
Cavallo et al. 2024 133.3 -46.002 0.484 – – –
Hunt & Reffert 2023 133.342 -46.039 0.484 -5.672 4.398 –
Castro-Ginard et al. 2022 133.32 -46.02 0.48 -5.67 4.38 –

💡 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 – – – – – 317* – –
Cavallo et al. 2024 2.47 3.05 – 6 0.240 – – –
Hunt & Reffert 2023 1.95 3.14 2.19 11 – – – –
Castro-Ginard et al. 2022 2.44 2.50 – 16 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 163 100.0 133.34 -46.04 0.49 -5.68 4.39 – 0.14

💡 Note: The % column shows the percentage of members that UBC 1447 shares with each listed object.

Visualization

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