Theia 200

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0.02 UTI
0.25
CN
0.14
Cdens
0.5
CC3
0.0
Clit
0.12
Cdup
Radius (P>50% members) 24.0 [arcmin]
  • CN 0.25 Poorly populated
  • Cdens 0.14 Very loose
  • CC3 0.5 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 0.12 Likely duplicate

Overview

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Theia 200 is a poorly populated, very loose object of intermediate C3 quality. Its parallax locates it at a close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age 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 Intermediate age

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 – 18.877 60.756 1.155 2.947 -1.691 -15.76
Hunt & Reffert 2024 18.701 60.75 1.148 2.959 -1.672 -14.795
Cavallo et al. 2024 19.113 60.914 1.148 – – –
Hunt & Reffert 2023 18.701 60.75 1.148 2.959 -1.672 -14.795

💡 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 – – – – – 75* – –
Cavallo et al. 2024 0.89 1.07 – 214 0.270 – – –
Hunt & Reffert 2023 0.83 0.89 0.27 155 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 378 88.0 19.01 60.83 1.15 2.94 -1.68 -14.02 0.15
CWNU 389 40.0 20.2 60.93 1.12 3.0 -1.7 -18.9 0.13

💡 Note: The % column shows the percentage of members that Theia 200 shares with each listed object.

Visualization

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