Theia 1890

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0.12 UTI
0.75
CN
0.92
Cdens
0.75
CC3
0.0
Clit
0.25
Cdup
Radius (P>50% members) 13.5 [arcmin]
  • CN 0.75 Rich
  • Cdens 0.92 Very dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 0.25 Possibly duplicate

Overview

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Theia 1890 is a rich, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by low 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 possibly a duplicate object, which shares a significant percentage of members with at least one previously reported entry. See table with shared members information.

Relatively close Low 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 – 127.514 -41.937 0.799 -5.408 5.005 24.152
Hunt & Reffert 2024 127.473 -41.914 0.778 -5.4 5.02 23.055
Cavallo et al. 2024 127.419 -41.868 0.793 – – –
Hunt & Reffert 2023 127.473 -41.914 0.778 -5.4 5.02 23.055

💡 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 – – – – – 347* – –
Cavallo et al. 2024 1.14 0.92 – 18 -0.020 – – –
Hunt & Reffert 2023 1.18 0.94 1.72 26 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 1030 74.8 127.59 -41.95 0.8 -5.39 4.96 24.15 0.49
CWWDL 13550 39.6 127.57 -41.94 0.8 -5.41 4.99 24.47 0.0

💡 Note: The % column shows the percentage of members that Theia 1890 shares with each listed object.

Visualization

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