Theia 2460

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0.08 UTI
0.71
CN
1.0
Cdens
0.75
CC3
0.0
Clit
0.16
Cdup
Radius (P>50% members) 7.4 [arcmin]
  • CN 0.71 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 0.16 Likely duplicate

Overview

â„šī¸
Theia 2460 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, below 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.

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 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 – 256.154 -51.388 0.888 -0.682 -1.246 1.932
Hunt & Reffert 2024 256.158 -51.401 0.879 -0.693 -1.267 9.52
Cavallo et al. 2024 256.144 -51.387 0.883 – – –
Hunt & Reffert 2023 256.158 -51.401 0.879 -0.693 -1.267 9.52

💡 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 – – – – – 315* – –
Cavallo et al. 2024 1.16 0.94 – 162 0.460 – – –
Hunt & Reffert 2023 1.07 0.82 0.48 157 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 1151 83.7 256.16 -51.39 0.89 -0.68 -1.24 1.93 0.48

💡 Note: The % column shows the percentage of members that Theia 2460 shares with each listed object.

Visualization

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