Theia 47

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0.30 UTI
0.46
CN
0.28
Cdens
0.25
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 25.5 [arcmin]
  • CN 0.46 Poorly populated
  • Cdens 0.28 Loose
  • CC3 0.25 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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Theia 47 is a poorly populated, loose object of low C3 quality. Its parallax locates it at a close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the age and metallicity parameters (see Parameters). It is poorly studied in the literature.

Note: This object shares a significant percentage of members with at least one entry reported in the same catalogue. See table with shared members information.

Close Moderate extinction Near-solar metallicity Young

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 – 64.207 51.455 1.285 0.442 -3.424 0.288
Zhang et al. 2024 63.989 51.598 – – – –
Cavallo et al. 2024 65.333 50.837 1.285 – – –
Hunt & Reffert 2023 63.989 51.598 1.283 0.329 -3.482 3.016
He et al. 2022 66.228 51.801 1.305 0.77 -3.86 –

💡 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] Bfr BSS
Zhang et al. 2024 – – – – -0.209* – – –
Cavallo et al. 2024 0.74 2.53 – 32 -0.790 – – –
Hunt & Reffert 2023 0.75 1.29 1.74 406 – – – –
He et al. 2022 – 2.20 – 50 – – – –

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 1125 54.3 64.52 51.16 1.28 0.44 -3.39 -1.3 0.16
HSC 1205 50.0 64.34 51.32 1.29 0.46 -3.32 -1.3 0.01

💡 Note: The % column shows the percentage of members that Theia 47 shares with each listed object.

Visualization

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