UBC 1020

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0.66 UTI
0.82
CN
1.0
Cdens
1.0
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 5.7 [arcmin]
  • CN 0.82 Rich
  • 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 1020 is a rich, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a massive, near-solar metallicity, young cluster (see Parameters). It is poorly studied in the literature.

Note: This object shares a small percentage of members with 4 later reported entries. See table with shared members information.

Relatively close High extinction Massive 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 – 277.259 -12.717 0.464 0.621 -1.65 10.831
Hunt & Reffert 2024 277.25 -12.71 0.454 0.622 -1.638 -6.17
Cavallo et al. 2024 277.258 -12.726 0.457 – – –
Hunt & Reffert 2023 277.25 -12.71 0.454 0.622 -1.638 -6.17
Castro-Ginard et al. 2022 277.26 -12.72 0.48 0.63 -1.66 17.71

💡 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 – – – – – 2739* – –
Cavallo et al. 2024 1.99 3.42 – 110 0.210 – – –
Hunt & Reffert 2023 1.99 3.21 2.72 82 – – – –
Castro-Ginard et al. 2022 2.32 2.39 – 56 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 506 22.5 277.25 -12.72 0.48 0.64 -1.67 17.92 0.0
CWNU 44 17.6 277.26 -12.72 0.47 0.61 -1.66 18.06 0.0
OC 0032 12.1 277.26 -12.73 0.48 0.62 -1.66 88.27 0.0
HSC 210 6.2 277.31 -12.7 0.57 0.55 -1.62 – 0.06

💡 Note: The % column shows the percentage of members that UBC 1020 shares with each listed object.

Visualization

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