Theia 3337

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0.03 UTI
0.31
CN
1.0
Cdens
0.75
CC3
0.0
Clit
0.06
Cdup
Radius (P>50% members) 4.1 [arcmin]
  • CN 0.31 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 0.06 Very likely duplicate

Overview

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Theia 3337 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.

âš ī¸ Warning: This is very likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

Relatively close Low extinction Near-solar metallicity Intermediate age

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 – 138.986 -44.865 0.555 -5.202 5.153 20.178
Hunt & Reffert 2024 139.002 -44.882 0.551 -5.213 5.163 20.199
Cavallo et al. 2024 138.979 -44.847 0.549 – – –
Hunt & Reffert 2023 139.002 -44.882 0.551 -5.213 5.163 20.199

💡 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 – – – – – 223* – –
Cavallo et al. 2024 1.61 0.64 – 219 -0.130 – – –
Hunt & Reffert 2023 1.73 0.78 0.38 41 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 535 93.5 138.99 -44.86 0.56 -5.2 5.15 20.18 0.0
CWWDL 13965 93.5 138.98 -44.85 0.55 -5.19 5.14 20.18 0.14
UBC 1586 93.5 138.99 -44.86 0.56 -5.2 5.15 20.18 0.36

💡 Note: The % column shows the percentage of members that Theia 3337 shares with each listed object.

Visualization

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