Theia 2360

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0.21 UTI
0.73
CN
1.0
Cdens
0.75
CC3
0.0
Clit
0.42
Cdup
Radius (P>50% members) 10.7 [arcmin]
  • CN 0.73 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 0.42 Possibly duplicate

Overview

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Theia 2360 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, young cluster (see Parameters). It was recently reported in the literature.

âš ī¸ Warning: This is possibly a duplicate object, which shares a significant percentage of members with at least one previously reported entry. See table with shared members information.

Relatively close Low 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 – 120.627 -39.625 0.939 -2.559 5.681 14.168
Hunt & Reffert 2024 120.603 -39.614 0.934 -2.569 5.638 15.779
Cavallo et al. 2024 120.625 -39.603 0.938 – – –
Hunt & Reffert 2023 120.603 -39.614 0.934 -2.569 5.638 15.779

💡 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 – – – – – 258* – –
Cavallo et al. 2024 1.10 0.91 – 87 0.190 – – –
Hunt & Reffert 2023 1.01 0.66 1.32 83 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
FoF 2287 58.3 120.63 -39.64 0.95 -2.54 5.7 14.17 0.56
OC 0447 46.9 120.66 -39.64 0.95 -2.54 5.71 14.18 0.0

💡 Note: The % column shows the percentage of members that Theia 2360 shares with each listed object.

Visualization

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