Theia 2730

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0.26 UTI
0.0
CN
0.68
Cdens
1.0
CC3
0.0
Clit
0.76
Cdup
Radius (P>50% members) 2.1 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.68 Moderately dense
  • CC3 1.0 Very high quality
  • Clit 0.0 Rarely studied
  • Cdup 0.76 Very likely unique

Overview

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Theia 2730 is a sparse, moderately dense object of very high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It was recently reported in the literature.

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

Distant High extinction Near-solar metallicity Young

Cavallo et al. (2024)
Bronze sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 242.095 -53.483 0.23 -3.334 -3.701 -51.716
Hunt & Reffert 2024 242.091 -53.503 0.236 -3.342 -3.699 -17.403
Cavallo et al. 2024 242.074 -53.476 0.236 – – –
Hunt & Reffert 2023 242.091 -53.503 0.236 -3.342 -3.699 -17.403

💡 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 – – – – – 832* – –
Cavallo et al. 2024 4.31 4.92 – 36 -0.310 – – –
Hunt & Reffert 2023 3.89 4.19 2.70 132 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 2741 24.0 242.0 -53.5 0.32 -3.32 -3.75 -30.39 0.06

💡 Note: The % column shows the percentage of members that Theia 2730 shares with each listed object.

Visualization

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