Theia 1654

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0.42 UTI
0.52
CN
0.96
Cdens
0.62
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 9.3 [arcmin]
  • CN 0.52 Moderately populated
  • Cdens 0.96 Very dense
  • CC3 0.62 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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Theia 1654 is a moderately populated, very dense object of intermediate C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It was recently reported in the literature.
Relatively close Moderate 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 – 106.273 -10.442 0.806 -3.134 0.717 38.824
Hunt & Reffert 2024 106.259 -10.382 0.8 -3.156 0.85 28.412
Cavallo et al. 2024 106.244 -10.884 0.807 – – –
Hunt & Reffert 2023 106.259 -10.382 0.8 -3.156 0.85 28.412

💡 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 – – – – – 81* – –
Cavallo et al. 2024 1.52 1.41 – 15 -0.020 – – –
Hunt & Reffert 2023 1.17 0.93 2.34 25 – – – –

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

Visualization

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