Theia 2122

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0.07 UTI
0.32
CN
1.0
Cdens
1.0
CC3
0.0
Clit
0.16
Cdup
Radius (P>50% members) 8.1 [arcmin]
  • CN 0.32 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.0 Rarely studied
  • Cdup 0.16 Likely duplicate

Overview

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Theia 2122 is a poorly populated, very dense object of very high C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a very metal-poor, 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 Moderate extinction Very metal-poor 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 – 262.266 -30.896 0.949 3.797 -0.287 -16.653
Hunt & Reffert 2024 262.27 -30.933 0.941 3.764 -0.298 -17.8
Cavallo et al. 2024 262.305 -30.927 0.944 – – –
Hunt & Reffert 2023 262.27 -30.933 0.941 3.764 -0.298 -17.8

💡 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 – – – – – 144* – –
Cavallo et al. 2024 0.83 1.50 – 417 -1.120 – – –
Hunt & Reffert 2023 1.00 0.53 0.44 444 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
UFMG 67 84.4 262.26 -30.89 0.95 3.8 -0.29 -16.65 0.45

💡 Note: The % column shows the percentage of members that Theia 2122 shares with each listed object.

Visualization

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