Theia 2110

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0.14 UTI
0.72
CN
1.0
Cdens
0.38
CC3
0.0
Clit
0.32
Cdup
Radius (P>50% members) 5.4 [arcmin]
  • CN 0.72 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 0.32 Possibly duplicate

Overview

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Theia 2110 is a moderately populated, very dense object of low C3 quality. Its parallax locates it at a moderate distance, above 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.

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 Moderate extinction Near-solar metallicity Young

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 – 113.856 -18.631 0.396 -1.75 2.407 122.744
Hunt & Reffert 2024 113.864 -18.642 0.394 -1.76 2.414 122.747
Cavallo et al. 2024 113.846 -18.603 0.394 – – –
Hunt & Reffert 2023 113.864 -18.642 0.394 -1.76 2.414 122.747

💡 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 – – – – – 542* – –
Cavallo et al. 2024 2.79 2.29 – 100 0.330 – – –
Hunt & Reffert 2023 2.23 1.90 2.36 63 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
DBSB 7 67.7 113.86 -18.64 0.39 -1.72 2.4 109.31 0.68
CWWDL 13798 44.1 113.86 -18.6 0.41 -1.74 2.41 – 0.09

💡 Note: The % column shows the percentage of members that Theia 2110 shares with each listed object.

Visualization

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