Theia 3428

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0.00 UTI
0.43
CN
1.0
Cdens
0.75
CC3
0.25
Clit
0.0
Cdup
Radius (P>50% members) 5.9 [arcmin]
  • CN 0.43 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 0.0 Very likely duplicate

Overview

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Theia 3428 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, below 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 – 90.319 4.565 0.717 0.479 -2.076 33.6
Zhang et al. 2024 90.301 4.602 – – – –
Hunt & Reffert 2024 90.301 4.602 0.707 0.465 -2.07 48.074
Cavallo et al. 2024 90.338 4.527 0.712 – – –
Hunt & Reffert 2023 90.301 4.602 0.707 0.465 -2.07 48.074

💡 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
Zhang et al. 2024 – – – – 0.001* – – –
Hunt & Reffert 2024 – – – – – 343* – –
Cavallo et al. 2024 1.43 2.00 – 282 0.300 – – –
Hunt & Reffert 2023 1.31 1.87 2.52 141 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 257 100.0 90.33 4.56 0.73 0.49 -2.06 39.31 0.2
UBC 1325 83.7 90.32 4.56 0.72 0.5 -2.08 23.35 0.42

💡 Note: The % column shows the percentage of members that Theia 3428 shares with each listed object.

Visualization

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