Theia 6

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0.03 UTI
0.51
CN
1.0
Cdens
1.0
CC3
0.0
Clit
0.06
Cdup
Radius (P>50% members) 7.0 [arcmin]
  • CN 0.51 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.0 Rarely studied
  • Cdup 0.06 Very likely duplicate

Overview

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Theia 6 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a low-mass, near-solar metallicity, very 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.

Close Moderate extinction Low mass Near-solar metallicity Very young

Cavallo et al. (2024)
Bronze sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 10.841 61.968 1.834 3.391 -2.19 -9.524
Hunt & Reffert 2024 10.877 61.975 1.823 3.312 -2.238 -2.089
Cavallo et al. 2024 10.114 62.04 1.838 – – –
Hunt & Reffert 2023 10.877 61.975 1.823 3.312 -2.238 -2.089

💡 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 – – – – – 40* – –
Cavallo et al. 2024 0.65 1.46 – 5 -0.100 – – –
Hunt & Reffert 2023 0.53 0.93 1.85 5 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 1040 94.2 10.84 61.96 1.84 3.36 -2.2 -9.52 0.5

💡 Note: The % column shows the percentage of members that Theia 6 shares with each listed object.

Visualization

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