Theia 3339

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0.01 UTI
0.0
CN
0.13
Cdens
0.38
CC3
0.0
Clit
0.12
Cdup
Radius (P>50% members) 9.7 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.13 Very loose
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 0.12 Likely duplicate

Overview

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Theia 3339 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by low 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 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 Low extinction Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as a moving group.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 123.355 -33.078 0.491 -2.203 1.339 28.852
Cavallo et al. 2024 123.322 -33.074 0.489 – – –
Hunt & Reffert 2023 123.413 -33.197 0.491 -2.214 1.365 –

💡 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
Cavallo et al. 2024 1.81 0.93 – 380 -0.030 – – –
Hunt & Reffert 2023 1.94 0.53 1.26 545 – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 1562 88.0 123.3 -33.03 0.49 -2.21 1.34 25.74 0.17

💡 Note: The % column shows the percentage of members that Theia 3339 shares with each listed object.

Visualization

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