UBC 274

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0.21 UTI
0.81
CN
0.29
Cdens
1.0
CC3
0.03
Clit
0.48
Cdup
Core radius and density 2.1 [pc], 1.4 [pc-2]
  • CN 0.81 Rich
  • Cdens 0.29 Loose
  • CC3 1.0 Very high quality
  • Clit 0.03 Rarely studied
  • Cdup 0.48 Possibly duplicate

Overview

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UBC 274 is a rich, loose object of very high C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by low 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 possibly a duplicate object, which shares a significant 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– 156.256 -72.558 0.52 -6.883 1.455 -23.512
Li et al. 2023 156.262 -72.549 0.53 -6.89 1.45 –
Castro-Ginard et al. 2020 156.194 -72.575 0.508 -6.882 1.445 –

💡 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– 1.845 0.835 – 1710 -0.140 – – 4
Li et al. 2023 2.00 0.35 – 2818 -0.140 – – 4(1)
Kounkel et al. 2020 1.69 1.32 – 603 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
FoF 5 52.4 156.14 -72.53 0.52 -6.88 1.47 -23.22 0.49
OC 0560 2.0 154.51 -72.17 0.52 -6.87 1.69 -22.78 0.05

💡 Note: The % column shows the percentage of members that UBC 274 shares with each listed object.

Visualization

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