Theia 85

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0.06 UTI
0.3
CN
1.0
Cdens
0.38
CC3
0.0
Clit
0.17
Cdup
Radius (P>50% members) 8.9 [arcmin]
  • CN 0.3 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 0.17 Likely duplicate

Overview

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Theia 85 is a poorly populated, very dense object of low C3 quality. Its parallax locates it at a close distance, above 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 likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

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 – 57.694 60.202 1.576 -2.995 -0.459 -22.247
Zhang et al. 2024 57.684 60.202 – – – –
Cavallo et al. 2024 58.114 59.798 1.583 – – –
Hunt & Reffert 2023 57.684 60.202 1.583 -3.058 -0.497 -22.462

💡 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 – – – – -0.282* – – –
Cavallo et al. 2024 0.59 0.69 – 46 -0.110 – – –
Hunt & Reffert 2023 0.60 0.82 0.56 58 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
OC 0264 83.3 57.69 60.17 1.58 -2.99 -0.51 -22.24 0.35
CWNU 149 80.0 57.66 60.16 1.58 -2.99 -0.51 -22.24 0.01

💡 Note: The % column shows the percentage of members that Theia 85 shares with each listed object.

Visualization

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