Theia 274

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0.07 UTI
0.63
CN
0.64
Cdens
1.0
CC3
0.0
Clit
0.16
Cdup
Radius (P>50% members) 22.0 [arcmin]
  • CN 0.63 Moderately populated
  • Cdens 0.64 Moderately dense
  • CC3 1.0 Very high quality
  • Clit 0.0 Rarely studied
  • Cdup 0.16 Likely duplicate

Overview

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Theia 274 is a moderately populated, moderately dense object of very high C3 quality. Its parallax locates it at a close distance, near 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 likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

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 – 128.46 -39.577 1.317 -8.108 5.645 28.014
Hunt & Reffert 2024 128.578 -39.522 1.301 -8.056 5.687 26.714
Cavallo et al. 2024 128.325 -39.818 1.302 – – –
Hunt & Reffert 2023 128.578 -39.522 1.301 -8.056 5.687 26.714

💡 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 – – – – – 481* – –
Cavallo et al. 2024 0.75 0.41 – 115 0.160 – – –
Hunt & Reffert 2023 0.73 0.21 1.10 125 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
Alessi Teutsch 7 84.2 128.23 -39.41 1.33 -8.11 5.64 28.72 0.8

💡 Note: The % column shows the percentage of members that Theia 274 shares with each listed object.

Visualization

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