UBC 117

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0.25 UTI
0.8
CN
1.0
Cdens
1.0
CC3
0.03
Clit
0.44
Cdup
Core radius and density 2.4 [pc], 5.2 [pc-2]
  • CN 0.8 Rich
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.03 Rarely studied
  • Cdup 0.44 Possibly duplicate

Overview

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UBC 117 is a rich, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate 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– 282.106 8.714 0.432 -0.082 -1.476 26.303
Li et al. 2023 282.109 8.72 0.43 -0.08 -1.48 –
Castro-Ginard et al. 2020 282.106 8.717 0.423 -0.071 -1.473 –

💡 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– 2.225 2.665 – 1780 0.097 – – 1
Li et al. 2023 2.00 1.85 – 3162 0.097 – – 1(1)
Kounkel et al. 2020 2.45 3.48 – 398 – – – –

(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 597 55.7 282.1 8.71 0.43 -0.06 -1.48 26.3 0.65
CWWDL 3112 54.5 282.11 8.71 0.43 -0.08 -1.48 27.58 0.0

💡 Note: The % column shows the percentage of members that UBC 117 shares with each listed object.

Visualization

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