Theia 2000

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0.40 UTI
0.39
CN
1.0
Cdens
0.62
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 6.9 [arcmin]
  • CN 0.39 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.62 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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Theia 2000 is a poorly populated, very dense object of intermediate C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It was recently reported in the literature.
Relatively close Low extinction Near-solar metallicity Very young

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 – 114.109 -25.377 0.732 -4.95 4.86 26.834
Hunt & Reffert 2024 114.132 -25.356 0.74 -4.903 4.888 32.455
Cavallo et al. 2024 114.02 -24.761 0.741 – – –
Hunt & Reffert 2023 114.132 -25.356 0.74 -4.903 4.888 32.455

💡 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 – – – – – 92* – –
Cavallo et al. 2024 1.45 0.63 – 12 -0.150 – – –
Hunt & Reffert 2023 1.27 0.38 1.75 21 – – – –

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

Visualization

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