Theia 2289

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0.12 UTI
0.72
CN
0.82
Cdens
0.75
CC3
0.0
Clit
0.27
Cdup
Radius (P>50% members) 10.0 [arcmin]
  • CN 0.72 Moderately populated
  • Cdens 0.82 Dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 0.27 Possibly duplicate

Overview

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Theia 2289 is a moderately populated, dense object of high 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, intermediate-age cluster (see Parameters). It was recently reported in the literature.

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

Relatively close Low 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 – 106.721 -12.276 0.611 -1.039 -0.255 18.255
Hunt & Reffert 2024 106.723 -12.251 0.614 -1.045 -0.251 18.251
Cavallo et al. 2024 106.725 -12.307 0.617 – – –
Hunt & Reffert 2023 106.723 -12.251 0.614 -1.045 -0.251 18.251

💡 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 – – – – – 338* – –
Cavallo et al. 2024 1.56 0.90 – 398 0.300 – – –
Hunt & Reffert 2023 1.54 0.84 1.02 196 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CMa23 73.1 106.71 -12.31 0.61 -1.03 -0.27 18.26 0.42
UBC 1363 49.5 106.7 -12.3 0.61 -1.04 -0.28 18.26 0.0

💡 Note: The % column shows the percentage of members that Theia 2289 shares with each listed object.

Visualization

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