Theia 3114

Click to load Aladin Lite
0.02 UTI
0.0
CN
0.3
Cdens
1.0
CC3
0.0
Clit
0.08
Cdup
Radius (P>50% members) 4.1 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.3 Loose
  • CC3 1.0 Very high quality
  • Clit 0.0 Rarely studied
  • Cdup 0.08 Very likely duplicate

Overview

â„šī¸
Theia 3114 is a sparse, 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, young 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 Moderate extinction Near-solar metallicity Young

Cavallo et al. (2024)
Gold sample.

Data

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 229.732 -60.0 0.304 -3.801 -2.987 -45.533
Hunt & Reffert 2024 229.71 -60.004 0.305 -3.8 -2.99 -45.529
Cavallo et al. 2024 229.753 -60.01 0.305 – – –
Hunt & Reffert 2023 229.71 -60.004 0.305 -3.8 -2.99 -45.529

💡 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 – – – – – 400* – –
Cavallo et al. 2024 2.21 2.63 – 98 0.020 – – –
Hunt & Reffert 2023 2.94 2.46 1.89 17 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 2285 92.0 229.73 -60.01 0.31 -3.81 -3.0 -45.53 0.31

💡 Note: The % column shows the percentage of members that Theia 3114 shares with each listed object.

Visualization

â„šī¸