Theia 3916

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0.20 UTI
0.56
CN
1.0
Cdens
0.75
CC3
0.0
Clit
0.43
Cdup
Radius (P>50% members) 11.3 [arcmin]
  • CN 0.56 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 0.43 Possibly duplicate

Overview

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Theia 3916 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.

âš ī¸ Warning: This is possibly a duplicate object, which shares a significant percentage of members with at least one previously reported entry. See table with shared members information.

Relatively close Moderate 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 – 315.098 38.991 0.963 -3.277 -8.965 -15.502
Hunt & Reffert 2024 315.091 39.002 0.947 -3.266 -8.916 -16.279
Cavallo et al. 2024 314.959 38.937 0.95 – – –
Hunt & Reffert 2023 315.091 39.002 0.947 -3.266 -8.916 -16.279

💡 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 – – – – – 179* – –
Cavallo et al. 2024 1.06 1.02 – 355 0.380 – – –
Hunt & Reffert 2023 1.01 1.09 1.48 142 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 1148 57.4 315.04 38.99 0.96 -3.27 -8.96 -14.92 0.31

💡 Note: The % column shows the percentage of members that Theia 3916 shares with each listed object.

Visualization

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