Theia 199

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0.06 UTI
0.44
CN
0.3
Cdens
0.75
CC3
0.0
Clit
0.2
Cdup
Radius (P>50% members) 22.9 [arcmin]
  • CN 0.44 Poorly populated
  • Cdens 0.3 Loose
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 0.2 Likely duplicate

Overview

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Theia 199 is a poorly populated, loose object of high 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.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 309.434 54.512 1.222 -3.096 -6.732 -20.545
Hunt & Reffert 2024 309.382 54.688 1.206 -3.098 -6.839 -24.486
Cavallo et al. 2024 309.22 53.817 1.211 – – –
Hunt & Reffert 2023 309.382 54.688 1.206 -3.098 -6.839 -24.486

💡 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 – – – – – 50* – –
Cavallo et al. 2024 0.84 0.68 – 44 0.260 – – –
Hunt & Reffert 2023 0.79 0.46 1.09 34 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 444 79.5 309.46 54.4 1.22 -3.11 -6.73 -20.54 0.28

💡 Note: The % column shows the percentage of members that Theia 199 shares with each listed object.

Visualization

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