Theia 3832

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0.21 UTI
0.52
CN
0.55
Cdens
0.75
CC3
0.0
Clit
0.57
Cdup
Radius (P>50% members) 3.9 [arcmin]
  • CN 0.52 Moderately populated
  • Cdens 0.55 Moderately dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 0.57 Likely unique

Overview

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Theia 3832 is a moderately populated, moderately 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, young cluster (see Parameters). It was recently reported in the literature.

Note: This is likely a unique object, which shares a moderate percentage of members with at least one previously reported entry. See table with shared members information.

Distant Moderate 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 – 3.722 62.822 0.255 -2.285 -0.723 -87.259
Hunt & Reffert 2024 3.726 62.818 0.262 -2.286 -0.713 -87.25
Cavallo et al. 2024 3.719 62.82 0.262 – – –
Hunt & Reffert 2023 3.726 62.818 0.262 -2.286 -0.713 -87.25

💡 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 – – – – – 477* – –
Cavallo et al. 2024 3.34 1.58 – 79 0.490 – – –
Hunt & Reffert 2023 3.59 1.71 1.87 53 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
UBC 1200 42.6 3.72 62.82 0.27 -2.28 -0.73 -87.26 0.28

💡 Note: The % column shows the percentage of members that Theia 3832 shares with each listed object.

Visualization

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