Theia 2266

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0.01 UTI
0.65
CN
1.0
Cdens
0.75
CC3
0.0
Clit
0.01
Cdup
Stellar density (N50/rad) 5.1 [N/pc2]
  • CN 0.65 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 0.01 Very likely duplicate

Overview

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Theia 2266 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, below 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.

âš ī¸ Warning: This is very likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

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– 102.728 -9.986 0.477 -1.297 1.241 –
Hunt & Reffert 2024 102.721 -10.015 0.468 -1.297 1.247 –
Cavallo et al. 2024 102.738 -9.977 0.471 – – –
Hunt & Reffert 2023 102.721 -10.015 0.468 -1.297 1.247 –

💡 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– 1.995 1.335 1.82 226 -0.040 430 – –
Hunt & Reffert 2024 – – – – – 430(1) – –
Cavallo et al. 2024 2.04 1.53 – 219 -0.040 – – –
Hunt & Reffert 2023 1.95 1.14 1.82 233 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
HXHWL 61 98.8 102.73 -9.97 0.48 -1.29 1.24 – 0.5
UBC 1354 77.5 102.73 -9.98 0.48 -1.3 1.24 – 0.0
CWWDL 13298 58.8 102.73 -9.98 0.47 -1.31 1.24 – 0.0

💡 Note: The % column shows the percentage of members that Theia 2266 shares with each listed object.

Visualization

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