Theia 5736

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0.06 UTI
0.0
CN
0.62
Cdens
0.75
CC3
0.25
Clit
0.16
Cdup
Radius (P>50% members) 5.1 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.62 Moderately dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 0.16 Likely duplicate

Overview

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Theia 5736 is a sparse, moderately dense object of high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by low 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 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 Low 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 – 75.847 40.553 0.546 1.601 -2.494 -6.261
Zhang et al. 2024 75.826 40.591 – – – –
Hunt & Reffert 2024 75.826 40.591 0.537 1.581 -2.455 -17.209
Cavallo et al. 2024 75.849 40.523 0.537 – – –
Hunt & Reffert 2023 75.826 40.591 0.537 1.581 -2.455 -17.209

💡 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 – – – – 0.011* – – –
Hunt & Reffert 2024 – – – – – 307* – –
Cavallo et al. 2024 1.78 0.77 – 158 0.170 – – –
Hunt & Reffert 2023 1.71 0.75 1.05 199 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
OC 0281 84.0 75.85 40.5 0.55 1.6 -2.5 -13.56 0.2

💡 Note: The % column shows the percentage of members that Theia 5736 shares with each listed object.

Visualization

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