Theia 1928

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0.00 UTI
0.5
CN
1.0
Cdens
0.75
CC3
0.0
Clit
0.0
Cdup
Radius (P>50% members) 3.7 [arcmin]
  • CN 0.5 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 0.0 Very likely duplicate

Overview

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Theia 1928 is a moderately populated, very dense object of high 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, intermediate-age 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 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 – 288.822 14.417 0.362 -1.704 -2.518 –
Hunt & Reffert 2024 288.83 14.442 0.371 -1.683 -2.514 8.19
Cavallo et al. 2024 288.815 14.411 0.369 – – –
Hunt & Reffert 2023 288.83 14.442 0.371 -1.683 -2.514 8.19

💡 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 – – – – – 402* – –
Cavallo et al. 2024 2.37 2.95 – 324 0.000 – – –
Hunt & Reffert 2023 2.50 2.90 1.21 155 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
PHOC 8 100.0 288.81 14.4 0.36 -1.71 -2.51 -9.55 0.47

💡 Note: The % column shows the percentage of members that Theia 1928 shares with each listed object.

Visualization

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