UBC 570

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0.03 UTI
0.9
CN
1.0
Cdens
1.0
CC3
0.03
Clit
0.06
Cdup
Core radius and density 1.1 [pc], 13 [pc-2]
  • CN 0.9 Very rich
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.03 Rarely studied
  • Cdup 0.06 Very likely duplicate

Overview

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UBC 570 is a very rich, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is rarely studied in the literature.

âš ī¸ Warning: This is very likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 267.676 -30.209 0.332 -0.106 -1.347 -7.854
Li et al. 2023 267.677 -30.213 0.33 -0.11 -1.33 –
Castro-Ginard et al. 2020 267.677 -30.198 0.313 -0.107 -1.342 –

💡 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– 2.15 2.0 – 662 -0.006 – – 0
Li et al. 2023 2.40 1.75 – 1000 -0.006 – – 0(1)
Kounkel et al. 2020 1.90 2.25 – 324 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
NGC 6451 94.5 267.68 -30.21 0.33 -0.1 -1.34 -7.85 0.98
OC 0703 8.1 267.67 -30.2 0.31 -0.14 -1.38 -8.52 0.0
OC 0702 0.6 267.67 -30.21 0.52 -0.12 -1.11 8.5 0.17

💡 Note: The % column shows the percentage of members that UBC 570 shares with each listed object.

Visualization

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