Theia 2096

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0.02 UTI
0.36
CN
1.0
Cdens
0.75
CC3
0.0
Clit
0.06
Cdup
Radius (P>50% members) 2.3 [arcmin]
  • CN 0.36 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 0.06 Very likely duplicate

Overview

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Theia 2096 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a metal-poor, young cluster (see Parameters). It was recently reported in the literature.

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

Relatively close High extinction Metal-poor Young

Cavallo et al. (2024)
Bronze sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 243.687 -51.584 0.349 -2.721 -4.435 -33.096
Hunt & Reffert 2024 243.704 -51.58 0.361 -2.752 -4.474 -35.792
Cavallo et al. 2024 243.699 -51.58 0.358 – – –
Hunt & Reffert 2023 243.704 -51.58 0.361 -2.752 -4.474 -35.792

💡 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 – – – – – 462* – –
Cavallo et al. 2024 2.99 4.06 – 48 -0.760 – – –
Hunt & Reffert 2023 2.51 3.03 2.60 108 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 1568 94.4 243.69 -51.58 0.35 -2.71 -4.43 -35.26 0.48

💡 Note: The % column shows the percentage of members that Theia 2096 shares with each listed object.

Visualization

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