Theia 1001

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0.31 UTI
0.75
CN
1.0
Cdens
0.75
CC3
0.25
Clit
0.52
Cdup
Radius (P>50% members) 7.2 [arcmin]
  • CN 0.75 Rich
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 0.52 Likely unique

Overview

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Theia 1001 is a rich, very dense object of high C3 quality. Its parallax locates it at a close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It was recently reported in the literature.

Note: This is likely a unique object, which shares a moderate percentage of members with at least one previously reported entry. See table with shared members information.

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 – 343.75 59.247 1.093 2.186 0.031 -17.51
Zhang et al. 2024 343.75 59.243 – – – –
Hunt & Reffert 2024 343.75 59.243 1.093 2.21 0.023 -19.092
Cavallo et al. 2024 343.767 59.255 1.096 – – –
Hunt & Reffert 2023 343.75 59.243 1.093 2.21 0.023 -19.092

💡 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
Zhang et al. 2024 – – – – -0.300* – – –
Hunt & Reffert 2024 – – – – – 258* – –
Cavallo et al. 2024 0.97 2.17 – 234 0.470 – – –
Hunt & Reffert 2023 0.88 2.34 1.78 105 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
UBC 394 48.5 343.79 59.24 1.09 2.18 0.02 -14.22 0.58

💡 Note: The % column shows the percentage of members that Theia 1001 shares with each listed object.

Visualization

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