Theia 4419

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0.02 UTI
0.38
CN
0.32
Cdens
0.75
CC3
0.0
Clit
0.05
Cdup
Radius (P>50% members) 4.6 [arcmin]
  • CN 0.38 Poorly populated
  • Cdens 0.32 Loose
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 0.05 Very likely duplicate

Overview

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Theia 4419 is a poorly populated, loose object of high 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 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.

Distant Low 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 – 115.321 -23.39 0.276 -2.551 3.774 –
Hunt & Reffert 2024 115.283 -23.382 0.269 -2.554 3.775 –
Cavallo et al. 2024 115.319 -23.425 0.269 – – –
Hunt & Reffert 2023 115.283 -23.382 0.269 -2.554 3.775 –

💡 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 – – – – – 351* – –
Cavallo et al. 2024 3.06 0.77 – 457 -0.040 – – –
Hunt & Reffert 2023 4.31 0.95 0.89 158 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 1403 94.7 115.34 -23.42 0.28 -2.55 3.77 – 0.3

💡 Note: The % column shows the percentage of members that Theia 4419 shares with each listed object.

Visualization

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