Theia 399

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0.15 UTI
0.0
CN
0.19
Cdens
0.38
CC3
0.1
Clit
1.0
Cdup
Core radius and density 1.3 [pc], 0.9 [pc-2]
  • CN 0.0 Sparse
  • Cdens 0.19 Very loose
  • CC3 0.38 Low quality
  • Clit 0.1 Rarely studied
  • Cdup 1.0 Unique

Overview

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Theia 399 is a sparse, very loose object of low C3 quality. Its parallax locates it at a close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, young 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.

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as moving group. CMD class: 0.95 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.95 (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– 93.616 17.411 1.667 -0.488 -4.522 17.828
Zhang et al. 2024 93.671 17.398 – – – –
Swiggum et al. 2024 93.671 17.398 1.669 -0.451 -4.559 17.139
Cavallo et al. 2024 93.296 17.651 1.684 – – –
Hunt & Reffert 2023 93.671 17.398 1.669 -0.451 -4.559 18.312
Kounkel & Covey 2019 92.842 17.008 1.478 – – 0.771

💡 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– 0.62 0.4 0.95 27 -0.015 138 – –
Zhang et al. 2024 – – – – -0.110(1) – – –
Swiggum et al. 2024 0.59 – – 27 – 138 – –
Cavallo et al. 2024 0.65 0.58 – 27 0.080 – – –
Hunt & Reffert 2023 0.58 0.24 0.95 27 – – – –
Kounkel & Covey 2019 0.68 0.40 – 136 – – – –

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

Visualization

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