UPK 300

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0.27 UTI
0.26
CN
0.2
Cdens
0.38
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 1.0 [N/pc2]
  • CN 0.26 Poorly populated
  • Cdens 0.2 Very loose
  • CC3 0.38 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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UPK 300 is a poorly populated, very loose object of low C3 quality. Its parallax locates it at a close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a metal-poor, young cluster (see Parameters). It is poorly studied in the literature.

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 99999– 57.759 60.121 1.052 0.185 -0.824 -9.115
Hunt & Reffert 2024 57.408 60.146 1.059 0.207 -0.768 -8.096
Cavallo et al. 2024 57.94 60.06 1.054 – – –
Hunt & Reffert 2023 57.408 60.146 1.059 0.207 -0.768 -8.096
Sim et al. 2019 58.02 59.983 – 0.25 -0.75 –

💡 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] Bfrac BSS
UCC 99999– 0.95 2.635 1.23 62 -0.620 87 – –
Hunt & Reffert 2024 – – – – – 87(1) – –
Cavallo et al. 2024 0.95 2.81 – 21 -0.620 – – –
Hunt & Reffert 2023 0.91 2.46 1.23 62 – – – –
Sim et al. 2019 0.96 – – 398 – – – –

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Visualization

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