Theia 780

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0.00 UTI
0.28
CN
0.61
Cdens
0.38
CC3
0.25
Clit
0.0
Cdup
Radius (P>50% members) 11.0 [arcmin]
  • CN 0.28 Poorly populated
  • Cdens 0.61 Moderately dense
  • CC3 0.38 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 0.0 Very likely duplicate

Overview

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Theia 780 is a poorly populated, moderately dense object of low C3 quality. Its parallax locates it at a 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 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.

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 – 81.669 30.344 1.052 -0.687 -4.481 3.743
Zhang et al. 2024 81.659 30.32 – – – –
Hunt & Reffert 2024 81.659 30.32 1.034 -0.618 -4.341 7.345
Cavallo et al. 2024 81.47 30.156 1.034 – – –
Hunt & Reffert 2023 81.659 30.32 1.034 -0.618 -4.341 7.345

💡 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 – – – – -0.165* – – –
Hunt & Reffert 2024 – – – – – 89* – –
Cavallo et al. 2024 0.93 0.85 – 89 -0.120 – – –
Hunt & Reffert 2023 0.91 0.59 0.97 232 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 1104 100.0 81.65 30.35 1.05 -0.67 -4.48 3.74 0.34

💡 Note: The % column shows the percentage of members that Theia 780 shares with each listed object.

Visualization

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