UBC 372

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0.10 UTI
0.68
CN
1.0
Cdens
1.0
CC3
0.38
Clit
0.14
Cdup
Radius (P>50% members) 2.1 [arcmin]
  • CN 0.68 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.38 Poorly studied
  • Cdup 0.14 Likely duplicate

Overview

â„šī¸
UBC 372 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 moderate extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is poorly studied in the literature.

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

Distant 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 – 302.38 38.291 0.271 -2.584 -4.875 –
Zhang et al. 2024 302.37 38.289 – – – –
Hunt & Reffert 2024 302.37 38.289 0.261 -2.595 -4.867 –
Cavallo et al. 2024 302.384 38.284 0.266 – – –
Hunt & Reffert 2023 302.37 38.289 0.261 -2.595 -4.867 –
Cantat-Gaudin et al. 2020 302.375 38.291 0.255 -2.601 -4.885 –
Castro-Ginard et al. 2020 302.368 38.283 0.261 -2.609 -4.891 –

💡 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
Zhang et al. 2024 – – – – 0.134* – – –
Hunt & Reffert 2024 – – – – – 566* – –
Cavallo et al. 2024 3.02 2.43 – 91 -0.100 – – –
Hunt & Reffert 2023 3.31 2.15 0.62 71 – – – –
Cantat-Gaudin et al. 2020 3.24 1.90 – 115 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
HXWHB 14 85.9 302.38 38.29 0.28 -2.6 -4.88 – 0.53

💡 Note: The % column shows the percentage of members that UBC 372 shares with each listed object.

Visualization

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