UBC 127

Click to load Aladin Lite
0.21 UTI
0.84
CN
1.0
Cdens
0.75
CC3
0.03
Clit
0.39
Cdup
Core radius and density 2.1 [pc], 10.0 [pc-2]
  • CN 0.84 Rich
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.03 Rarely studied
  • Cdup 0.39 Possibly duplicate

Overview

â„šī¸
UBC 127 is a rich, very dense object of 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, 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

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 296.389 21.154 0.449 -0.369 -3.571 -18.114
Li et al. 2023 296.397 21.162 0.45 -0.35 -3.57 –
Castro-Ginard et al. 2020 296.384 21.157 0.436 -0.35 -3.551 –

💡 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– 2.45 2.88 – 2514 0.097 – – 2
Li et al. 2023 2.40 2.05 – 4467 0.097 – – 2(1)
Kounkel et al. 2020 2.50 3.71 – 562 – – – –

(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 321 60.7 296.39 21.15 0.45 -0.36 -3.57 -18.19 0.61
OC 0085 12.0 296.4 21.17 0.46 -0.38 -3.54 -18.05 0.0

💡 Note: The % column shows the percentage of members that UBC 127 shares with each listed object.

Visualization

â„šī¸