Theia 3524

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0.05 UTI
0.29
CN
0.33
Cdens
0.5
CC3
0.0
Clit
0.21
Cdup
Radius (P>50% members) 9.7 [arcmin]
  • CN 0.29 Poorly populated
  • Cdens 0.33 Loose
  • CC3 0.5 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 0.21 Likely duplicate

Overview

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Theia 3524 is a poorly populated, loose object of intermediate 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 – 115.546 -21.984 0.676 -2.498 1.721 34.458
Hunt & Reffert 2024 115.674 -22.105 0.665 -2.484 1.732 39.656
Cavallo et al. 2024 115.535 -21.964 0.667 – – –
Hunt & Reffert 2023 115.674 -22.105 0.665 -2.484 1.732 39.656

💡 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 – – – – – 141* – –
Cavallo et al. 2024 1.49 0.60 – 126 0.060 – – –
Hunt & Reffert 2023 1.41 0.17 0.47 265 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWWDL 14179 79.3 115.54 -21.87 0.68 -2.51 1.71 39.8 0.03
HXHWL 43 65.5 115.48 -21.85 0.67 -2.5 1.69 40.05 0.27

💡 Note: The % column shows the percentage of members that Theia 3524 shares with each listed object.

Visualization

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