Theia 67

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0.00 UTI
0.52
CN
1.0
Cdens
0.62
CC3
0.0
Clit
0.0
Cdup
Radius (P>50% members) 74.2 [arcmin]
  • CN 0.52 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 0.62 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 0.0 Very likely duplicate

Overview

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Theia 67 is a moderately populated, very dense object of intermediate C3 quality. Its parallax locates it at a very 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 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.

Very close Low extinction Near-solar metallicity Young

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 – 259.964 -24.956 6.753 -4.613 -21.651 -3.451
Cavallo et al. 2024 259.763 -25.058 6.756 – – –
Hunt & Reffert 2023 260.336 -25.059 6.753 -4.668 -21.781 -3.663

💡 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 0.15 1.03 – 38 0.190 – – –
Hunt & Reffert 2023 0.14 0.27 0.45 12 – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
OCSN 1 100.0 259.77 -24.91 6.73 -4.72 -21.59 -3.5 0.42

💡 Note: The % column shows the percentage of members that Theia 67 shares with each listed object.

Visualization

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