UBC 1032

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0.45 UTI
0.0
CN
1.0
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 5.0 [N/pc2]
  • CN 0.0 Sparse
  • 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 1032 is a sparse, very dense object of high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is poorly studied in the literature.

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 99999– 279.573 -9.279 0.293 -1.456 -3.086 19.605
Hunt & Reffert 2024 279.575 -9.274 0.29 -1.435 -3.05 –
Cavallo et al. 2024 279.573 -9.27 0.287 – – –
Hunt & Reffert 2023 279.575 -9.274 0.29 -1.435 -3.05 –
Castro-Ginard et al. 2022 279.57 -9.27 0.29 -1.47 -3.1 –

💡 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– 3.12 3.72 2.24 33 -0.270 522 – –
Hunt & Reffert 2024 – – – – – 522(1) – –
Cavallo et al. 2024 2.73 3.72 – 46 -0.270 – – –
Hunt & Reffert 2023 3.12 3.89 2.24 28 – – – –
Castro-Ginard et al. 2022 3.60 3.01 – 33 – – – –

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

Visualization

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