Theia 1645

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0.04 UTI
0.44
CN
0.75
Cdens
0.75
CC3
0.0
Clit
0.09
Cdup
Radius (P>50% members) 10.4 [arcmin]
  • CN 0.44 Poorly populated
  • Cdens 0.75 Dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 0.09 Very likely duplicate

Overview

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Theia 1645 is a poorly populated, dense object of high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, very 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 Very 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 – 262.752 -33.48 0.883 2.507 -1.917 -4.183
Hunt & Reffert 2024 262.758 -33.468 0.89 2.436 -1.936 -4.202
Cavallo et al. 2024 262.653 -33.534 0.891 – – –
Hunt & Reffert 2023 262.758 -33.468 0.89 2.436 -1.936 -4.202

💡 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 – – – – – 325* – –
Cavallo et al. 2024 0.99 1.66 – 9 -0.200 – – –
Hunt & Reffert 2023 1.06 1.57 1.87 16 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
UFMG 77 90.9 262.79 -33.47 0.88 2.51 -1.9 0.07 0.46
CWWDL 14393 81.8 262.72 -33.48 0.89 2.47 -1.91 0.07 0.08

💡 Note: The % column shows the percentage of members that Theia 1645 shares with each listed object.

Visualization

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