Theia 3127

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0.30 UTI
0.57
CN
0.19
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 17.8 [arcmin]
  • CN 0.57 Moderately populated
  • Cdens 0.19 Very loose
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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Theia 3127 is a moderately populated, very loose object of high C3 quality. Its parallax locates it at a relatively close distance, near 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.

Note: This object shares a moderate percentage of members with a later 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 – 144.748 -54.07 0.627 -8.215 5.795 -3.15
Hunt & Reffert 2024 144.753 -54.071 0.623 -8.236 5.762 -2.065
Cavallo et al. 2024 145.197 -54.28 0.625 – – –
Hunt & Reffert 2023 144.753 -54.071 0.623 -8.236 5.762 -2.065

💡 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 – – – – – 87* – –
Cavallo et al. 2024 1.57 0.40 – 331 0.460 – – –
Hunt & Reffert 2023 1.51 0.50 0.46 300 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3635 40.6 144.74 -54.09 0.62 -8.2 5.82 – 0.0

💡 Note: The % column shows the percentage of members that Theia 3127 shares with each listed object.

Visualization

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