UBC 1450

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0.55 UTI
0.48
CN
1.0
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 3.1 [arcmin]
  • CN 0.48 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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UBC 1450 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the age parameter (see Parameters). It is poorly studied in the literature.

Note: This object shares a large percentage of members with 2 later reported entries. See table with shared members information.

Relatively close Moderate extinction Near-solar metallicity 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 – 129.99 -48.229 0.461 -4.994 5.085 35.403
Hunt & Reffert 2024 129.993 -48.225 0.455 -4.995 5.062 35.575
Cavallo et al. 2024 129.984 -48.236 0.457 – – –
Hunt & Reffert 2023 129.993 -48.225 0.455 -4.995 5.062 35.575
Castro-Ginard et al. 2022 130.0 -48.24 0.46 -5.01 5.08 –

💡 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 – – – – – 222* – –
Cavallo et al. 2024 1.80 1.05 – 372 0.210 – – –
Hunt & Reffert 2023 2.00 1.28 1.18 75 – – – –
Castro-Ginard et al. 2022 2.33 1.19 – 45 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 242 100.0 129.99 -48.23 0.45 -4.99 5.07 23.01 0.1
CWWDL 168 91.7 129.99 -48.23 0.46 -4.98 5.08 23.01 0.0

💡 Note: The % column shows the percentage of members that UBC 1450 shares with each listed object.

Visualization

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