Theia 2356

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0.00 UTI
0.38
CN
0.82
Cdens
0.5
CC3
0.0
Clit
0.0
Cdup
Radius (P>50% members) 8.3 [arcmin]
  • CN 0.38 Poorly populated
  • Cdens 0.82 Dense
  • CC3 0.5 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 0.0 Very likely duplicate

Overview

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Theia 2356 is a poorly populated, dense object of intermediate C3 quality. Its parallax locates it at a relatively close 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.

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 – 98.025 0.469 0.795 1.44 -1.347 23.135
Hunt & Reffert 2024 98.005 0.476 0.785 1.432 -1.319 22.233
Cavallo et al. 2024 98.035 0.444 0.792 – – –
Hunt & Reffert 2023 98.005 0.476 0.785 1.432 -1.319 22.233

💡 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 – – – – – 186* – –
Cavallo et al. 2024 1.35 1.38 – 398 0.220 – – –
Hunt & Reffert 2023 1.18 1.35 0.85 233 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
HXHWL 19 100.0 98.03 0.44 0.8 1.44 -1.33 23.14 0.41

💡 Note: The % column shows the percentage of members that Theia 2356 shares with each listed object.

Visualization

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