Theia 253

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0.14 UTI
0.64
CN
0.89
Cdens
0.75
CC3
0.0
Clit
0.31
Cdup
Radius (P>50% members) 33.8 [arcmin]
  • CN 0.64 Moderately populated
  • Cdens 0.89 Dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 0.31 Possibly duplicate

Overview

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Theia 253 is a moderately populated, dense object of high C3 quality. Its parallax locates it at a very close distance, above the mid-plane, affected by low extinction. It is catalogued as a low-mass, near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.

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

Very close Low extinction Low mass 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 – 293.629 32.11 2.348 2.443 -1.329 -19.421
Hunt & Reffert 2024 293.685 32.122 2.363 2.35 -1.32 -19.223
Cavallo et al. 2024 293.546 32.186 2.367 – – –
Hunt & Reffert 2023 293.685 32.122 2.363 2.35 -1.32 -19.223

💡 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 – – – – – 43* – –
Cavallo et al. 2024 0.43 0.51 – 66 0.120 – – –
Hunt & Reffert 2023 0.40 0.16 0.45 137 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 347 69.2 293.63 32.16 2.38 2.53 -1.31 -20.97 0.45
CWWDL 14662 39.7 293.7 32.1 2.41 2.68 -1.33 -20.77 0.0

💡 Note: The % column shows the percentage of members that Theia 253 shares with each listed object.

Visualization

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