Theia 240

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0.35 UTI
0.0
CN
1.0
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad) 6.4 [N/pc2]
  • CN 0.0 Sparse
  • 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 240 is a sparse, very dense object of high C3 quality. Its parallax locates it at a very 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.

Palma et al. (2025)
Classified as optical pair P575, along with Theia_828.

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 99999– 279.283 -20.38 2.433 -0.027 -4.909 -12.611
Hunt & Reffert 2024 279.192 -20.357 2.387 0.056 -4.837 -13.036
Cavallo et al. 2024 279.093 -20.055 2.394 – – –
Hunt & Reffert 2023 279.192 -20.357 2.387 0.056 -4.837 -13.036

💡 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] Bfrac BSS
UCC 99999– 0.41 1.3 0.74 68 -0.190 54 – –
Hunt & Reffert 2024 – – – – – 54(1) – –
Cavallo et al. 2024 0.42 1.60 – 25 -0.190 – – –
Hunt & Reffert 2023 0.40 1.00 0.74 110 – – – –

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Visualization

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