Theia 1871

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0.09 UTI
0.39
CN
1.0
Cdens
0.75
CC3
0.0
Clit
0.2
Cdup
Radius (P>50% members) 3.2 [arcmin]
  • CN 0.39 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 0.2 Likely duplicate

Overview

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Theia 1871 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 moderate extinction. It is catalogued as a metal-poor, young cluster (see Parameters). It was recently reported in the literature.

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

(*): The parallax distance estimate (~2.99 kpc) differs significantly from the median photometric distance (~2.20 kpc).

Relatively close Moderate extinction Metal-poor Young

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 – 273.52 -19.011 0.334 -0.391 -1.194 -6.44
Hunt & Reffert 2024 273.555 -18.985 0.333 -0.385 -1.206 -35.903
Cavallo et al. 2024 273.508 -19.019 0.332 – – –
Hunt & Reffert 2023 273.555 -18.985 0.333 -0.385 -1.206 -35.903

💡 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 – – – – – 674* – –
Cavallo et al. 2024 1.65 2.05 – 78 -0.520 – – –
Hunt & Reffert 2023 2.75 1.70 1.94 98 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
UBC 1009 79.5 273.51 -19.03 0.33 -0.35 -1.19 1.49 0.38

💡 Note: The % column shows the percentage of members that Theia 1871 shares with each listed object.

Visualization

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