Theia 4013

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0.24 UTI
0.52
CN
0.78
Cdens
1.0
CC3
0.0
Clit
0.53
Cdup
Radius (P>50% members) 4.3 [arcmin]
  • CN 0.52 Moderately populated
  • Cdens 0.78 Dense
  • CC3 1.0 Very high quality
  • Clit 0.0 Rarely studied
  • Cdup 0.53 Likely unique

Overview

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Theia 4013 is a moderately populated, dense object of very high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age 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.

Relatively close Moderate extinction Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Silver sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 278.005 -13.392 0.338 -0.796 -2.815 30.77
Hunt & Reffert 2024 277.998 -13.386 0.329 -0.773 -2.791 8.907
Cavallo et al. 2024 278.0 -13.405 0.331 – – –
Hunt & Reffert 2023 277.998 -13.386 0.329 -0.773 -2.791 8.907

💡 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 – – – – – 566* – –
Cavallo et al. 2024 2.16 2.48 – 115 0.040 – – –
Hunt & Reffert 2023 2.67 2.36 1.95 121 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 2920 47.2 278.01 -13.39 0.34 -0.8 -2.82 25.62 0.33

💡 Note: The % column shows the percentage of members that Theia 4013 shares with each listed object.

Visualization

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