Theia 2450

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0.06 UTI
0.62
CN
1.0
Cdens
1.0
CC3
0.0
Clit
0.12
Cdup
Radius (P>50% members) 10.3 [arcmin]
  • CN 0.62 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.0 Rarely studied
  • Cdup 0.12 Likely duplicate

Overview

â„šī¸
Theia 2450 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a relatively close distance, above 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 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

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 202.756 -57.163 0.872 -5.66 -1.375 -24.904
Hunt & Reffert 2024 202.849 -57.199 0.868 -5.649 -1.375 -23.524
Cavallo et al. 2024 202.784 -57.202 0.875 – – –
Hunt & Reffert 2023 202.849 -57.199 0.868 -5.649 -1.375 -23.524

💡 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 – – – – – 220* – –
Cavallo et al. 2024 1.15 1.22 – 26 0.130 – – –
Hunt & Reffert 2023 1.08 0.82 1.24 41 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 315 87.7 202.71 -57.17 0.88 -5.67 -1.37 -22.48 0.47
CWWDL 14467 79.5 202.71 -57.17 0.88 -5.66 -1.37 -29.46 0.0

💡 Note: The % column shows the percentage of members that Theia 2450 shares with each listed object.

Visualization

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