UBC 1190

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0.19 UTI
0.52
CN
0.85
Cdens
0.75
CC3
0.25
Clit
0.36
Cdup
Radius (P>50% members) 4.4 [arcmin]
  • CN 0.52 Moderately populated
  • Cdens 0.85 Dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 0.36 Possibly duplicate

Overview

UBC 1190 is a moderately populated, dense object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane. It is catalogued as a metal-rich, young cluster (see Parameters). It is poorly studied in the literature.

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.

Data

Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 358.913 60.858 0.363 -1.769 -1.062
Hunt & Reffert 2024 358.894 60.871 0.352 -1.764 -1.064
Cavallo et al. 2024 358.925 60.878 0.352
Hunt & Reffert 2023 358.894 60.871 0.352 -1.764 -1.064
Castro-Ginard et al. 2022 358.89 60.86 0.36 -1.79 -1.06

💡 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] Bfr BSS
Hunt & Reffert 2024 356*
Cavallo et al. 2024 2.92 1.87 174 0.570
Hunt & Reffert 2023 2.59 1.86 0.77 74
Castro-Ginard et al. 2022 2.91 1.58 61

💡 Note: The parameters are sometimes transformed from their original values to match the format of the columns shown here, see FAQ. The columns DAv, Bfr, BSS correspond to differential extinction, binary fraction, and blue stragglers, respectively. BSS values can be listed as fractions or integers.
(*): indicates that this parameter is assigned more than one value in the corresponding reference.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
HXHWL 4 64.2 358.94 60.86 0.36 -1.77 -1.05 0.38

💡 Note: The % column shows the percentage of members that UBC 1190 shares with each listed object.

Visualization

Galactocentric position diagram

💡 Note: How are the galactocentric plots generated? See FAQ.