Theia 2007

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0.04 UTI
0.0
CN
0.19
Cdens
0.38
CC3
0.0
Clit
0.32
Cdup
Radius (P>50% members) 10.4 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.19 Very loose
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 0.32 Possibly duplicate

Overview

â„šī¸
Theia 2007 is a sparse, very loose object of low C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young 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.

Relatively close Moderate extinction Near-solar metallicity Young

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 – 303.426 34.463 0.623 -0.877 -3.641 -36.821
Hunt & Reffert 2024 303.374 34.247 0.619 -0.856 -3.631 -36.69
Cavallo et al. 2024 303.391 34.422 0.62 – – –
Hunt & Reffert 2023 303.374 34.247 0.619 -0.856 -3.631 -36.69

💡 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 – – – – – 150* – –
Cavallo et al. 2024 1.67 1.47 – 100 0.420 – – –
Hunt & Reffert 2023 1.54 1.57 1.29 36 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 202 68.0 303.49 34.56 0.62 -0.84 -3.64 -24.64 0.22

💡 Note: The % column shows the percentage of members that Theia 2007 shares with each listed object.

Visualization

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