Theia 2921

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0.03 UTI
0.25
CN
0.38
Cdens
0.62
CC3
0.0
Clit
0.12
Cdup
Radius (P>50% members) 9.4 [arcmin]
  • CN 0.25 Poorly populated
  • Cdens 0.38 Loose
  • CC3 0.62 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 0.12 Likely duplicate

Overview

â„šī¸
Theia 2921 is a poorly populated, loose object of intermediate C3 quality. Its parallax locates it at a relatively close distance, near 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 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 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 – 294.856 23.733 0.756 -0.589 -3.626 -20.229
Hunt & Reffert 2024 294.802 23.803 0.761 -0.578 -3.655 -15.365
Cavallo et al. 2024 294.865 23.685 0.769 – – –
Hunt & Reffert 2023 294.802 23.803 0.761 -0.578 -3.655 -15.365

💡 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 – – – – – 80* – –
Cavallo et al. 2024 1.43 1.98 – 47 0.390 – – –
Hunt & Reffert 2023 1.27 1.84 0.79 84 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 373 88.0 294.91 23.66 0.76 -0.58 -3.63 -20.23 0.26

💡 Note: The % column shows the percentage of members that Theia 2921 shares with each listed object.

Visualization

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