Theia 2493

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0.02 UTI
0.36
CN
0.56
Cdens
0.38
CC3
0.25
Clit
0.06
Cdup
Radius (P>50% members) 5.2 [arcmin]
  • CN 0.36 Poorly populated
  • Cdens 0.56 Moderately dense
  • CC3 0.38 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 0.06 Very likely duplicate

Overview

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Theia 2493 is a poorly populated, moderately dense object of low 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, but with a large variance across recent sources for the metallicity parameter (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.

Relatively 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 – 61.693 48.858 0.423 0.392 -0.984 -48.044
Zhang et al. 2024 61.705 48.842 – – – –
Hunt & Reffert 2024 61.705 48.842 0.426 0.369 -0.995 –
Cavallo et al. 2024 61.569 48.85 0.423 – – –
Hunt & Reffert 2023 61.705 48.842 0.426 0.369 -0.995 –

💡 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
Zhang et al. 2024 – – – – -0.309* – – –
Hunt & Reffert 2024 – – – – – 266* – –
Cavallo et al. 2024 2.42 2.21 – 229 0.590 – – –
Hunt & Reffert 2023 2.22 2.31 1.89 114 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 1381 94.4 61.69 48.87 0.43 0.39 -0.99 -48.04 0.25

💡 Note: The % column shows the percentage of members that Theia 2493 shares with each listed object.

Visualization

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