Theia 1822

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0.10 UTI
0.64
CN
1.0
Cdens
0.75
CC3
0.0
Clit
0.22
Cdup
Radius (P>50% members) 5.1 [arcmin]
  • CN 0.64 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 0.22 Likely duplicate

Overview

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Theia 1822 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, near 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 – 252.881 -44.493 0.414 -0.597 -2.528 -80.971
Hunt & Reffert 2024 252.894 -44.496 0.419 -0.605 -2.523 -48.574
Cavallo et al. 2024 252.891 -44.496 0.419 – – –
Hunt & Reffert 2023 252.894 -44.496 0.419 -0.605 -2.523 -48.574

💡 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 – – – – – 719* – –
Cavallo et al. 2024 2.01 2.04 – 98 0.410 – – –
Hunt & Reffert 2023 2.14 2.14 2.64 85 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
UBC 1559 78.2 252.87 -44.49 0.41 -0.61 -2.54 -82.92 0.46

💡 Note: The % column shows the percentage of members that Theia 1822 shares with each listed object.

Visualization

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