Theia 5

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0.00 UTI
0.36
CN
1.0
Cdens
1.0
CC3
0.0
Clit
0.0
Cdup
Radius (P>50% members) 3.5 [arcmin]
  • CN 0.36 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.0 Rarely studied
  • Cdup 0.0 Very likely duplicate

Overview

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Theia 5 is a poorly populated, very dense object of very high C3 quality. Its parallax locates it at a very close distance, above 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.

Very 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 – 315.427 68.148 2.918 7.488 -1.403 -21.365
Hunt & Reffert 2024 315.432 68.153 2.912 7.906 -1.131 -20.132
Cavallo et al. 2024 318.327 68.853 2.913 – – –
Hunt & Reffert 2023 315.432 68.153 2.912 7.906 -1.131 -20.132

💡 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 – – – – – 43* – –
Cavallo et al. 2024 0.40 1.94 – 11 0.300 – – –
Hunt & Reffert 2023 0.33 0.81 1.80 9 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
OCSN 34 100.0 315.44 68.16 2.91 7.44 -1.39 -21.36 0.11
NGC 7023 94.4 316.35 68.5 2.91 7.83 -1.1 -13.98 0.54

💡 Note: The % column shows the percentage of members that Theia 5 shares with each listed object.

Visualization

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