Theia 181

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0.06 UTI
0.38
CN
0.32
Cdens
0.5
CC3
0.0
Clit
0.26
Cdup
Radius (P>50% members) 30.2 [arcmin]
  • CN 0.38 Poorly populated
  • Cdens 0.32 Loose
  • CC3 0.5 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 0.26 Possibly duplicate

Overview

â„šī¸
Theia 181 is a poorly populated, loose object of intermediate C3 quality. Its parallax locates it at a close distance, below 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 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 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 – 234.453 -64.678 1.806 -4.007 -5.33 10.824
Hunt & Reffert 2024 234.546 -64.857 1.789 -4.007 -5.276 8.726
Cavallo et al. 2024 234.232 -64.845 1.794 – – –
Hunt & Reffert 2023 234.546 -64.857 1.789 -4.007 -5.276 8.726

💡 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 0.55 0.38 – 135 0.310 – – –
Hunt & Reffert 2023 0.53 0.23 0.77 112 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWWDL 14599 73.7 235.32 -64.36 1.82 -3.98 -5.4 10.59 0.35

💡 Note: The % column shows the percentage of members that Theia 181 shares with each listed object.

Visualization

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