Theia 7

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0.21 UTI
0.64
CN
1.0
Cdens
1.0
CC3
0.0
Clit
0.4
Cdup
Radius (P>50% members) 96.9 [arcmin]
  • CN 0.64 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.0 Rarely studied
  • Cdup 0.4 Possibly duplicate

Overview

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Theia 7 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a very close distance, near the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the metallicity parameter (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.

Very close High extinction Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Wood 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 – 68.628 24.719 7.676 6.71 -21.199 13.002
Zhang et al. 2024 68.304 24.39 – – – –
Cavallo et al. 2024 68.497 24.686 7.696 – – –
Hunt & Reffert 2023 68.304 24.39 7.674 6.85 -21.316 14.217

💡 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
Zhang et al. 2024 – – – – -0.288* – – –
Cavallo et al. 2024 0.15 3.84 – 32 0.300 – – –
Hunt & Reffert 2023 0.13 3.44 2.10 187 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
OCSN 52 60.3 68.73 24.35 7.74 7.0 -21.17 14.64 0.48
Taurus 3.8 65.78 27.29 7.72 8.8 -25.91 14.81 0.38

💡 Note: The % column shows the percentage of members that Theia 7 shares with each listed object.

Visualization

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