Theia 3118

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0.11 UTI
0.52
CN
0.46
Cdens
1.0
CC3
0.0
Clit
0.28
Cdup
Radius (P>50% members) 5.4 [arcmin]
  • CN 0.52 Moderately populated
  • Cdens 0.46 Loose
  • CC3 1.0 Very high quality
  • Clit 0.0 Rarely studied
  • Cdup 0.28 Possibly duplicate

Overview

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Theia 3118 is a moderately populated, loose object of very high C3 quality. Its parallax locates it at a moderate* distance, below the mid-plane, affected by moderate 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.

(*): The parallax distance estimate (~3.06 kpc) differs significantly from the median photometric distance (~2.35 kpc).

Relatively close Moderate 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 – 239.78 -55.819 0.327 -2.589 -2.942 -7.782
Hunt & Reffert 2024 239.805 -55.87 0.329 -2.617 -2.981 -29.422
Cavallo et al. 2024 239.773 -55.816 0.33 – – –
Hunt & Reffert 2023 239.805 -55.87 0.329 -2.617 -2.981 -29.422

💡 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 – – – – – 829* – –
Cavallo et al. 2024 2.04 2.31 – 148 -0.120 – – –
Hunt & Reffert 2023 2.67 2.20 2.26 54 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
UFMG 45 71.7 239.71 -55.81 0.33 -2.58 -2.9 -24.95 0.52

💡 Note: The % column shows the percentage of members that Theia 3118 shares with each listed object.

Visualization

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