UBC 1150

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0.55 UTI
0.5
CN
1.0
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 2.0 [arcmin]
  • CN 0.5 Moderately 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 1150 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by moderate 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 Moderate extinction Near-solar metallicity Very young

Cavallo et al. (2024)
Silver sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 319.5 60.08 0.624 -4.642 -3.476 -21.773
Hunt & Reffert 2024 319.499 60.081 0.626 -4.644 -3.511 -21.745
Cavallo et al. 2024 319.488 60.09 0.633 – – –
Hunt & Reffert 2023 319.499 60.081 0.626 -4.644 -3.511 -21.745
Castro-Ginard et al. 2022 319.49 60.09 0.63 -4.69 -3.52 –

💡 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 – – – – – 281* – –
Cavallo et al. 2024 1.75 2.01 – 9 0.190 – – –
Hunt & Reffert 2023 1.51 2.12 2.18 4 – – – –
Castro-Ginard et al. 2022 1.52 2.04 – 14 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 309 92.2 319.5 60.08 0.62 -4.63 -3.5 -21.77 0.02

💡 Note: The % column shows the percentage of members that UBC 1150 shares with each listed object.

Visualization

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