Theia 12

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0.20 UTI
0.67
CN
1.0
Cdens
0.75
CC3
0.0
Clit
0.42
Cdup
Radius (P>50% members) 17.6 [arcmin]
  • CN 0.67 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 0.42 Possibly duplicate

Overview

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Theia 12 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a close distance, near the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It was recently reported in the literature.

âš ī¸ Warning: This is possibly a duplicate object, which shares a significant percentage of members with at least one previously reported entry. See table with shared members information.

Close High extinction Near-solar metallicity Very young

Cavallo et al. (2024)
Silver sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 281.947 -2.396 1.584 0.222 -6.238 6.148
Hunt & Reffert 2024 282.102 -2.382 1.569 0.139 -6.178 6.12
Cavallo et al. 2024 281.825 -2.246 1.571 – – –
Hunt & Reffert 2023 282.102 -2.382 1.569 0.139 -6.178 6.12

💡 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 – – – – – 262* – –
Cavallo et al. 2024 0.69 3.85 – 7 0.080 – – –
Hunt & Reffert 2023 0.61 3.19 2.91 5 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 1245 58.3 282.06 -2.44 1.59 0.31 -6.31 5.34 0.41
Ryu 269 10.7 282.18 -2.46 1.6 0.31 -6.01 43.62 0.3

💡 Note: The % column shows the percentage of members that Theia 12 shares with each listed object.

Visualization

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