Theia 696

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0.13 UTI
0.27
CN
0.08
Cdens
0.25
CC3
0.03
Clit
1.0
Cdup
Core radius and density 3.4 [pc], 0.4 [pc-2]
  • CN 0.27 Poorly populated
  • Cdens 0.08 Very loose
  • CC3 0.25 Low quality
  • Clit 0.03 Rarely studied
  • Cdup 1.0 Unique

Overview

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Theia 696 is a poorly populated, very loose object of low C3 quality. Its parallax locates it at a very close distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is rarely studied in the literature.

Note: This object shares a significant percentage of members with a later reported entry. See table with shared members information.

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.

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as moving group. CMD class: 0.79 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.79 (50th percentile).

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 272.251 -73.605 3.376 1.427 -14.676 20.297
Cavallo et al. 2024 272.784 -73.828 3.466 – – –
Hunt & Reffert 2023 271.719 -73.993 3.459 1.344 -14.992 15.632
Kounkel & Covey 2019 272.758 -72.364 2.946 – – 10.872

💡 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– 0.3 0.55 0.35 157 -0.010 – – –
Cavallo et al. 2024 0.30 0.55 – 76 -0.010 – – –
Hunt & Reffert 2023 0.28 0.11 0.35 157 – – – –
Kounkel & Covey 2019 0.34 0.61 – 325 – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 1180 51.9 272.05 -74.33 3.38 1.79 -14.41 20.24 0.03

💡 Note: The % column shows the percentage of members that Theia 696 shares with each listed object.

Visualization

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