Theia 1829

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0.01 UTI
0.25
CN
0.99
Cdens
0.5
CC3
0.0
Clit
0.04
Cdup
Radius (P>50% members) 7.3 [arcmin]
  • CN 0.25 Poorly populated
  • Cdens 0.99 Very dense
  • CC3 0.5 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 0.04 Very likely duplicate

Overview

â„šī¸
Theia 1829 is a poorly populated, very dense object of intermediate C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a metal-poor, intermediate-age 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.

Close Moderate extinction Metal-poor 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 – 278.19 -13.003 0.947 0.623 -3.792 -16.499
Hunt & Reffert 2024 278.214 -13.019 0.945 0.618 -3.807 -8.878
Cavallo et al. 2024 278.207 -13.041 0.949 – – –
Hunt & Reffert 2023 278.214 -13.019 0.945 0.618 -3.807 -8.878

💡 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 – – – – – 119* – –
Cavallo et al. 2024 0.84 1.41 – 195 -0.550 – – –
Hunt & Reffert 2023 1.01 1.12 0.46 126 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWWDL 14361 96.0 278.18 -13.02 0.95 0.62 -3.8 -15.24 0.33

💡 Note: The % column shows the percentage of members that Theia 1829 shares with each listed object.

Visualization

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