Theia 2665

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0.01 UTI
0.34
CN
0.33
Cdens
0.25
CC3
0.0
Clit
0.06
Cdup
Radius (P>50% members) 10.3 [arcmin]
  • CN 0.34 Poorly populated
  • Cdens 0.33 Loose
  • CC3 0.25 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 0.06 Very likely duplicate

Overview

â„šī¸
Theia 2665 is a poorly populated, loose object of low 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-poor, 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 Metal-poor 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 – 335.467 55.908 0.657 -1.579 -1.094 -29.005
Hunt & Reffert 2024 335.446 55.939 0.667 -1.561 -1.117 -25.241
Cavallo et al. 2024 335.474 55.915 0.663 – – –
Hunt & Reffert 2023 335.446 55.939 0.667 -1.561 -1.117 -25.241

💡 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 – – – – – 123* – –
Cavallo et al. 2024 1.28 1.35 – 257 -0.570 – – –
Hunt & Reffert 2023 1.45 0.85 0.23 284 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 2458 94.1 335.49 55.91 0.65 -1.58 -1.09 -22.09 0.3

💡 Note: The % column shows the percentage of members that Theia 2665 shares with each listed object.

Visualization

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