UBC 1592

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0.58 UTI
0.65
CN
1.0
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 5.3 [arcmin]
  • CN 0.65 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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UBC 1592 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is poorly studied in the literature.

Note: This object shares a significant percentage of members with a later reported entry. See table with shared members information.

Close Low extinction Near-solar metallicity Young

Cavallo et al. (2024)
Gold sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 213.608 -64.195 1.098 -4.479 -4.327 -9.557
Hunt & Reffert 2024 213.573 -64.19 1.09 -4.498 -4.313 -7.017
Cavallo et al. 2024 213.592 -64.189 1.091 – – –
Hunt & Reffert 2023 213.573 -64.19 1.09 -4.498 -4.313 -7.017
Castro-Ginard et al. 2022 213.59 -64.19 1.08 -4.51 -4.29 –

💡 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 – – – – – 292* – –
Cavallo et al. 2024 0.91 0.71 – 166 0.440 – – –
Hunt & Reffert 2023 0.87 0.80 0.43 56 – – – –
Castro-Ginard et al. 2022 0.98 0.68 – 99 – – – –

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 261 57.5 213.61 -64.2 1.09 -4.48 -4.34 -9.5 0.0

💡 Note: The % column shows the percentage of members that UBC 1592 shares with each listed object.

Visualization

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