Theia 4725

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0.06 UTI
0.3
CN
0.75
Cdens
0.62
CC3
0.0
Clit
0.17
Cdup
Radius (P>50% members) 3.3 [arcmin]
  • CN 0.3 Poorly populated
  • Cdens 0.75 Dense
  • CC3 0.62 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 0.17 Likely duplicate

Overview

â„šī¸
Theia 4725 is a poorly populated, dense object of intermediate C3 quality. Its parallax locates it at a moderate 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 – 301.609 36.418 0.339 -2.542 -5.103 –
Hunt & Reffert 2024 301.612 36.431 0.313 -2.547 -5.089 –
Cavallo et al. 2024 301.532 36.281 0.319 – – –
Hunt & Reffert 2023 301.612 36.431 0.313 -2.547 -5.089 –

💡 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 – – – – – 234* – –
Cavallo et al. 2024 2.98 2.43 – 60 0.090 – – –
Hunt & Reffert 2023 2.81 2.17 2.35 45 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
OC 0103 83.3 301.61 36.42 0.35 -2.54 -5.11 – 0.18
UBC 1091 56.7 301.61 36.37 0.34 -2.53 -5.11 – 0.24

💡 Note: The % column shows the percentage of members that Theia 4725 shares with each listed object.

Visualization

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