UBC 567

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0.00 UTI
1.0
CN
1.0
Cdens
1.0
CC3
0.03
Clit
0.0
Cdup
Core radius and density 1.7 [pc], 12 [pc-2]
  • CN 1.0 Very rich
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.03 Rarely studied
  • Cdup 0.0 Very likely duplicate

Overview

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UBC 567 is a very 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 near-solar metallicity, old 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.

Note: This object contains blue stragglers according to at least one source.

Castro-Ginard et al. (2020)
Coincidence with Sim et al. (2019, J. Korean Astron. Soc., 52, 145) or Liu & Pang (2019ApJS..245...32L), see Sect. 4.1.5.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 264.917 -33.224 0.355 0.141 -0.736 9.755
Li et al. 2023 264.914 -33.231 0.36 0.14 -0.76 –
Castro-Ginard et al. 2020 264.921 -33.214 0.36 0.168 -0.703 –

💡 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– 2.135 3.08 – 1654 0.097 – – 1
Li et al. 2023 2.00 2.55 – 2818 0.097 – – 1(1)
Kounkel et al. 2020 2.27 3.61 – 490 – – – –

(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 6404 100.0 264.91 -33.23 0.35 0.14 -0.74 9.75 0.92

💡 Note: The % column shows the percentage of members that UBC 567 shares with each listed object.

Visualization

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