Theia 3995

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0.25 UTI
0.26
CN
0.23
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 3.0 [arcmin]
  • CN 0.26 Poorly populated
  • Cdens 0.23 Very loose
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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Theia 3995 is a poorly populated, very loose object of high C3 quality. Its parallax locates it at a large distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.

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

Very distant Low extinction Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Gold sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 116.802 -25.231 0.182 -2.125 3.493 105.742
Hunt & Reffert 2024 116.829 -25.242 0.178 -2.119 3.498 105.701
Cavallo et al. 2024 116.799 -25.213 0.179 – – –
Hunt & Reffert 2023 116.829 -25.242 0.178 -2.119 3.498 105.701

💡 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
Hunt & Reffert 2024 – – – – – 150* – –
Cavallo et al. 2024 4.61 1.13 – 51 -0.070 – – –
Hunt & Reffert 2023 5.42 0.50 1.00 303 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 4632 84.6 116.79 -25.21 0.18 -2.11 3.5 105.74 0.08

💡 Note: The % column shows the percentage of members that Theia 3995 shares with each listed object.

Visualization

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