Theia 2254

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0.05 UTI
0.3
CN
1.0
Cdens
0.75
CC3
0.0
Clit
0.13
Cdup
Radius (P>50% members) 4.7 [arcmin]
  • CN 0.3 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 0.13 Likely duplicate

Overview

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Theia 2254 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a metal-rich, young cluster (see Parameters). It was recently reported in the literature.

âš ī¸ Warning: This is 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 Metal-rich 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 – 34.325 60.267 0.653 -0.93 0.104 34.063
Hunt & Reffert 2024 34.31 60.234 0.644 -0.904 0.113 34.064
Cavallo et al. 2024 34.354 60.259 0.648 – – –
Hunt & Reffert 2023 34.31 60.234 0.644 -0.904 0.113 34.064

💡 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 – – – – – 180* – –
Cavallo et al. 2024 1.67 2.10 – 54 0.690 – – –
Hunt & Reffert 2023 1.46 1.88 0.52 108 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
HXHWL 63 86.7 34.33 60.27 0.64 -0.89 0.11 34.06 0.41

💡 Note: The % column shows the percentage of members that Theia 2254 shares with each listed object.

Visualization

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