Theia 401

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0.13 UTI
0.0
CN
0.11
Cdens
0.5
CC3
0.03
Clit
1.0
Cdup
Stellar density (N50/rad) 0.5 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.11 Very loose
  • CC3 0.5 Intermediate quality
  • Clit 0.03 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
Theia 401 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a close distance, below the mid-plane, affected by low extinction. It is catalogued as a low-mass, near-solar metallicity, intermediate-age cluster (see Parameters). It is rarely studied 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.

Hunt & Reffert (2024)
Classified as open cluster. CMD class: 1.00 (50th percentile).

Hunt & Reffert (2023)
Classified as moving group. CMD class: 1.00 (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– 347.858 47.656 1.469 -0.874 -3.466 -9.281
Zhang et al. 2024 347.809 47.781 – – – –
Hunt & Reffert 2024 347.809 47.781 1.473 -0.781 -3.521 -7.645
Kounkel & Covey 2019 349.908 47.983 1.446 – – -1.639

💡 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– 0.69 0.42 – 157 -0.147 46 – –
Zhang et al. 2024 – – – – -0.147(1) – – –
Hunt & Reffert 2024 – – – – – 46(1) – –
Kounkel & Covey 2019 0.69 0.42 – 157 – – – –

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

Visualization

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