Theia 3229

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0.03 UTI
0.49
CN
1.0
Cdens
0.5
CC3
0.0
Clit
0.08
Cdup
Radius (P>50% members) 5.9 [arcmin]
  • CN 0.49 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.5 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 0.08 Very likely duplicate

Overview

â„šī¸
Theia 3229 is a poorly populated, very dense object of intermediate C3 quality. Its parallax locates it at a relatively close distance, above 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 very likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

Relatively 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 – 116.309 -20.045 0.611 -1.004 0.618 -6.159
Hunt & Reffert 2024 116.272 -20.04 0.601 -0.993 0.602 -6.158
Cavallo et al. 2024 116.316 -20.077 0.599 – – –
Hunt & Reffert 2023 116.272 -20.04 0.601 -0.993 0.602 -6.158

💡 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 – – – – – 291* – –
Cavallo et al. 2024 1.61 0.87 – 316 0.040 – – –
Hunt & Reffert 2023 1.57 0.79 0.41 321 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
HXHWL 24 91.8 116.32 -20.07 0.6 -1.01 0.62 -6.16 0.37

💡 Note: The % column shows the percentage of members that Theia 3229 shares with each listed object.

Visualization

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