Theia 383

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0.44 UTI
0.52
CN
0.42
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 2.1 [N/pc2]
  • CN 0.52 Moderately populated
  • Cdens 0.42 Loose
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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Theia 383 is a moderately populated, loose object of high C3 quality. Its parallax locates it at a very close distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It is poorly studied in the literature.

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

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as a moving group.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 113.243 0.005 2.137 -1.757 -0.222 1.54
Zhang et al. 2024 113.165 0.323 – – – –
Cavallo et al. 2024 113.239 -0.461 2.11 – – –
Hunt & Reffert 2023 113.165 0.323 2.103 -1.736 -0.086 0.533
He et al. 2022 113.19 0.191 2.147 -1.761 -0.3 –

💡 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– 0.475 0.3 0.53 219 0.138 – – –
Zhang et al. 2024 – – – – -0.095(1) – – –
Cavallo et al. 2024 0.50 0.30 – 219 0.370 – – –
Hunt & Reffert 2023 0.45 0.11 0.53 139 – – – –
He et al. 2022 – 0.40 – 282 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
OCSN 73 74.1 113.23 0.14 2.14 -1.76 -0.29 1.43 0.01

💡 Note: The % column shows the percentage of members that Theia 383 shares with each listed object.

Visualization

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