Theia 177

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0.12 UTI
0.0
CN
0.22
Cdens
0.38
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 29.2 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.22 Very loose
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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Theia 177 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, young cluster (see Parameters). It was recently reported in the literature.

âš ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Close Low extinction Near-solar metallicity Young

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 – 99.67 -45.134 1.875 -5.752 9.348 25.445
Cavallo et al. 2024 100.645 -46.305 1.837 – – –
Hunt & Reffert 2023 99.609 -45.134 1.836 -5.916 9.31 25.421

💡 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 0.58 0.46 – 13 0.000 – – –
Hunt & Reffert 2023 0.53 0.07 0.47 34 – – – –

Visualization

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