Theia 649

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0.07 UTI
0.0
CN
0.12
Cdens
0.25
CC3
0.0
Clit
0.96
Cdup
Radius (P>50% members) 31.5 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.12 Very loose
  • CC3 0.25 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 0.96 Unique

Overview

â„šī¸
Theia 649 is a sparse, very loose object of low C3 quality. Its parallax locates it at a close distance, below 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.

Note: This is a unique object, which shares a very small percentage of members with at least one previously reported entry. See table with shared members information.

âš ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=0.96) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Close Low extinction Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as a moving group.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 112.559 -51.369 1.529 -4.386 8.451 12.832
Cavallo et al. 2024 111.03 -51.659 1.576 – – –
Hunt & Reffert 2023 112.775 -51.328 1.573 -4.37 8.422 14.448

💡 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
Cavallo et al. 2024 0.63 0.45 – 148 0.290 – – –
Hunt & Reffert 2023 0.61 0.19 0.68 128 – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 270 4.0 109.02 -52.22 1.68 -4.24 8.6 15.02 0.07

💡 Note: The % column shows the percentage of members that Theia 649 shares with each listed object.

Visualization

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