Theia 1875

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0.03 UTI
0.0
CN
0.16
Cdens
0.75
CC3
0.0
Clit
0.16
Cdup
Radius (P>50% members) 7.7 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.16 Very loose
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 0.16 Likely duplicate

Overview

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Theia 1875 is a sparse, very loose object of high C3 quality. Its parallax locates it at a moderate 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 – 257.686 -41.504 0.416 -0.748 -2.714 -12.721
Hunt & Reffert 2024 257.632 -41.615 0.414 -0.75 -2.721 –
Cavallo et al. 2024 257.637 -41.627 0.414 – – –
Hunt & Reffert 2023 257.632 -41.615 0.414 -0.75 -2.721 –

💡 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 – – – – – 294* – –
Cavallo et al. 2024 1.87 2.83 – 29 0.130 – – –
Hunt & Reffert 2023 2.42 2.76 0.35 13 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWWDL 944 84.0 257.88 -41.36 0.42 -0.75 -2.72 -20.1 0.07
CWNU 85 56.0 257.92 -41.33 0.42 -0.73 -2.7 -17.36 0.65

💡 Note: The % column shows the percentage of members that Theia 1875 shares with each listed object.

Visualization

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