UBC 576

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0.64 UTI
0.35
CN
1.0
Cdens
0.75
CC3
0.55
Clit
1.0
Cdup
Radius (P>50% members) 3.0 [arcmin]
  • CN 0.35 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.55 Moderately studied
  • Cdup 1.0 Unique

Overview

â„šī¸
UBC 576 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by high 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 moderately studied in the literature.
Relatively close High extinction Near-solar metallicity Young

Almeida et al. (2025)
Mass determination: intermediate fit. Isochrone match: intermediate fit.

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 – 284.692 0.422 0.755 -0.712 -3.615 41.416
Almeida et al. 2025 284.704 0.417 – – – –
Hunt & Reffert 2024 284.694 0.432 0.755 -0.704 -3.623 32.711
Cavallo et al. 2024 284.693 0.4 0.755 – – –
Hunt & Reffert 2023 284.694 0.432 0.755 -0.704 -3.623 32.711
Almeida et al. 2023 284.694 0.4 – – – –
Dias et al. 2021 284.704 0.417 0.729 -0.737 -3.582 –
Cantat-Gaudin et al. 2020 284.685 0.433 0.744 -0.754 -3.55 –
Castro-Ginard et al. 2020 284.68 0.415 0.744 -0.745 -3.559 –

💡 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
Almeida et al. 2025 1.33 2.96 – 25 – 175 – –
Hunt & Reffert 2024 – – – – – 250* – –
Cavallo et al. 2024 1.11 3.47 – 145 -0.280 – – –
Hunt & Reffert 2023 1.27 3.32 2.27 104 – – – –
Almeida et al. 2023 1.28 3.05 – 26 0.018 180* 0.53 –
Tarricq et al. 2022 1.27 – – 87 – – – –
Dias et al. 2021 1.33 2.96 – 25 0.099 – – –
Cantat-Gaudin et al. 2020 1.32 2.48 – 78 – – – –

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

Visualization

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