UBC 1542

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0.60 UTI
0.52
CN
1.0
Cdens
1.0
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 3.0 [arcmin]
  • CN 0.52 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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UBC 1542 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, 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 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 – 240.107 -51.203 0.38 -1.225 -2.148 -37.362
Hunt & Reffert 2024 240.107 -51.205 0.398 -1.204 -2.157 -4.561
Cavallo et al. 2024 240.104 -51.201 0.397 – – –
Hunt & Reffert 2023 240.107 -51.205 0.398 -1.204 -2.157 -4.561
Castro-Ginard et al. 2022 240.08 -51.21 0.37 -1.17 -2.16 –

💡 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 – – – – – 753* – –
Cavallo et al. 2024 2.21 3.80 – 40 0.290 – – –
Hunt & Reffert 2023 2.33 3.60 1.19 89 – – – –
Castro-Ginard et al. 2022 3.39 3.55 – 17 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 142 87.0 240.1 -51.21 0.38 -1.22 -2.15 -42.62 0.01

💡 Note: The % column shows the percentage of members that UBC 1542 shares with each listed object.

Visualization

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