Theia 4007

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0.06 UTI
0.0
CN
0.15
Cdens
0.5
CC3
0.25
Clit
0.28
Cdup
Stellar density (N50/rad) 0.8 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.15 Very loose
  • CC3 0.5 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 0.28 Possibly duplicate

Overview

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Theia 4007 is a sparse, very 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 possibly a duplicate object, which shares a significant percentage of members with at least one previously reported entry. See table with shared members information.

Palma et al. (2025)
Classified as optical pair P581, along with Theia_3986.

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 99999– 323.839 49.578 0.543 -2.844 -4.517 –
Zhang et al. 2024 323.761 49.615 – – – –
Hunt & Reffert 2024 323.761 49.615 0.546 -2.795 -4.499 -40.819
Cavallo et al. 2024 323.812 49.582 0.542 – – –
Hunt & Reffert 2023 323.761 49.615 0.546 -2.795 -4.499 -40.819

💡 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] Bfrac BSS
UCC 99999– 1.745 0.66 0.27 520 -0.006 63 – –
Zhang et al. 2024 – – – – -0.153(1) – – –
Hunt & Reffert 2024 – – – – – 63(1) – –
Cavallo et al. 2024 1.75 0.76 – 407 0.140 – – –
Hunt & Reffert 2023 1.74 0.56 0.27 632 – – – –

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 1545 72.0 323.88 49.6 0.53 -2.88 -4.55 – 0.12

💡 Note: The % column shows the percentage of members that Theia 4007 shares with each listed object.

Visualization

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