Theia 71

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0.26 UTI
0.28
CN
0.29
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 79.3 [arcmin]
  • CN 0.28 Poorly populated
  • Cdens 0.29 Loose
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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Theia 71 is a poorly populated, loose object of high C3 quality. Its parallax locates it at a very 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 metallicity parameter (see Parameters). It was recently reported in the literature.

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

Very 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 – 68.561 20.384 5.243 4.136 -6.511 15.034
Zhang et al. 2024 68.582 20.467 – – – –
Cavallo et al. 2024 68.82 20.485 5.286 – – –
Hunt & Reffert 2023 68.582 20.467 5.286 4.091 -6.783 12.667

💡 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 – – – – 0.073* – – –
Cavallo et al. 2024 0.18 1.43 – 44 0.380 – – –
Hunt & Reffert 2023 0.19 0.71 0.45 16 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
HSC 1390 3.6 66.8 18.56 4.41 4.0 -8.1 17.55 0.13

💡 Note: The % column shows the percentage of members that Theia 71 shares with each listed object.

Visualization

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