Theia 4

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0.47 UTI
0.75
CN
1.0
Cdens
0.75
CC3
0.0
Clit
0.94
Cdup
Radius (P>50% members) 12.2 [arcmin]
  • CN 0.75 Rich
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 0.94 Very likely unique

Overview

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Theia 4 is a rich, very dense object of high C3 quality. Its parallax locates it at a close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It was recently reported in the literature.

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

Close Moderate extinction Near-solar metallicity Very 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 – 344.354 62.994 1.163 -2.404 -2.559 -13.562
Hunt & Reffert 2024 344.129 62.977 1.156 -2.397 -2.547 -17.247
Cavallo et al. 2024 344.419 63.037 1.154 – – –
Hunt & Reffert 2023 344.129 62.977 1.156 -2.397 -2.547 -17.247

💡 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 – – – – – 175* – –
Cavallo et al. 2024 0.87 2.09 – 5 -0.140 – – –
Hunt & Reffert 2023 0.83 2.03 1.47 5 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
FSR 0413 5.6 345.14 62.89 1.05 -2.24 -2.56 2.42 0.38

💡 Note: The % column shows the percentage of members that Theia 4 shares with each listed object.

Visualization

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