Theia 2621

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0.01 UTI
0.0
CN
0.24
Cdens
0.5
CC3
0.0
Clit
0.04
Cdup
Radius (P>50% members) 12.8 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.24 Very loose
  • CC3 0.5 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 0.04 Very likely duplicate

Overview

â„šī¸
Theia 2621 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by low 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 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 Low 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 – 123.368 -22.033 0.898 -1.166 0.366 3.837
Hunt & Reffert 2024 123.274 -22.006 0.892 -1.188 0.393 8.548
Cavallo et al. 2024 123.386 -22.169 0.892 – – –
Hunt & Reffert 2023 123.274 -22.006 0.892 -1.188 0.393 8.548

💡 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 – – – – – 69* – –
Cavallo et al. 2024 1.08 0.19 – 214 -0.080 – – –
Hunt & Reffert 2023 1.06 0.08 0.38 111 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 290 96.0 123.37 -22.02 0.9 -1.16 0.36 3.84 0.15

💡 Note: The % column shows the percentage of members that Theia 2621 shares with each listed object.

Visualization

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