Theia 1694

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0.22 UTI
0.0
CN
0.34
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad) 1.7 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.34 Loose
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
Theia 1694 is a sparse, loose object of high C3 quality. Its parallax locates it at a relatively close* distance, near the mid-plane, affected by high extinction. It is catalogued as a very metal-poor, young cluster (see Parameters). It was recently reported in the literature.

(*): The parallax distance estimate (~1.58 kpc) differs significantly from the median photometric distance (~2.33 kpc).

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)
Bronze sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 275.069 -14.934 0.631 0.055 -2.021 –
Hunt & Reffert 2024 275.082 -15.018 0.636 0.042 -2.029 -0.795
Cavallo et al. 2024 275.06 -14.811 0.635 – – –
Hunt & Reffert 2023 275.082 -15.018 0.636 0.042 -2.029 -0.795

💡 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– 2.335 3.15 2.31 22 -1.950 202 – –
Hunt & Reffert 2024 – – – – – 202(1) – –
Cavallo et al. 2024 3.19 3.53 – 18 -1.950 – – –
Hunt & Reffert 2023 1.48 2.77 2.31 27 – – – –

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Visualization

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