Theia 2443

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0.42 UTI
0.34
CN
1.0
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 8.4 [arcmin]
  • CN 0.34 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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Theia 2443 is a poorly populated, very dense object of high 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, intermediate-age cluster (see Parameters). It was recently reported in the literature.
Close Moderate 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 – 242.209 -56.046 0.985 -0.397 -4.061 -30.492
Hunt & Reffert 2024 242.231 -56.063 0.995 -0.449 -4.092 -12.173
Cavallo et al. 2024 242.052 -56.063 0.998 – – –
Hunt & Reffert 2023 242.231 -56.063 0.995 -0.449 -4.092 -12.173

💡 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 – – – – – 217* – –
Cavallo et al. 2024 0.86 1.23 – 324 -0.490 – – –
Hunt & Reffert 2023 0.95 0.83 1.08 71 – – – –

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

Visualization

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