UBC 335

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0.27 UTI
0.9
CN
1.0
Cdens
1.0
CC3
0.03
Clit
0.46
Cdup
Core radius and density 1.9 [pc], 7.1 [pc-2]
  • CN 0.9 Very rich
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.03 Rarely studied
  • Cdup 0.46 Possibly duplicate

Overview

â„šī¸
UBC 335 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 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 possibly a duplicate object, which shares a significant percentage of members with at least one previously reported entry. See table with shared members information.

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– 266.575 -29.175 0.483 1.718 -0.794 -34.637
Li et al. 2023 266.573 -29.163 0.48 1.72 -0.79 –
Castro-Ginard et al. 2020 266.557 -29.184 0.486 1.706 -0.765 –

💡 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– 1.625 2.375 – 776 0.097 – – 0
Li et al. 2023 2.19 1.75 – 1413 0.097 – – 0(1)
Kounkel et al. 2020 1.06 3.00 – 138 – – – –

(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 1624 54.0 266.58 -29.17 0.48 1.72 -0.79 -34.94 0.57
CWWDL 1660 43.0 266.57 -29.17 0.48 1.7 -0.8 -34.92 0.0
OC 0704 7.9 266.58 -29.18 0.49 1.72 -0.79 -34.16 0.0
Ryu 534 3.4 266.38 -29.08 0.5 1.78 -0.82 -36.72 0.14

💡 Note: The % column shows the percentage of members that UBC 335 shares with each listed object.

Visualization

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