Theia 872

Click to load Aladin Lite
0.13 UTI
0.0
CN
0.25
Cdens
0.38
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 18.8 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.25 Loose
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
Theia 872 is a sparse, loose object of low C3 quality. Its parallax locates it at a 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: 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 Moderate extinction Near-solar metallicity Young

Cavallo et al. (2024)
Silver sample.

Data

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 18.133 63.892 1.343 -1.43 0.326 -27.169
Hunt & Reffert 2024 18.64 63.879 1.331 -1.423 0.318 -30.294
Cavallo et al. 2024 17.906 63.945 1.345 – – –
Hunt & Reffert 2023 18.64 63.879 1.331 -1.423 0.318 -30.294

💡 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 – – – – – 63* – –
Cavallo et al. 2024 0.88 1.23 – 91 0.390 – – –
Hunt & Reffert 2023 0.72 1.72 1.19 56 – – – –

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

Visualization

â„šī¸