Theia 2615

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0.03 UTI
0.0
CN
0.43
Cdens
0.38
CC3
0.0
Clit
0.16
Cdup
Radius (P>50% members) 3.0 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.43 Loose
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 0.16 Likely duplicate

Overview

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Theia 2615 is a sparse, loose object of low C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate 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 likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

Distant 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 – 96.6 8.218 0.274 0.173 -1.777 46.5
Hunt & Reffert 2024 96.608 8.223 0.275 0.146 -1.747 –
Cavallo et al. 2024 96.589 8.247 0.269 – – –
Hunt & Reffert 2023 96.608 8.223 0.275 0.146 -1.747 –

💡 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 – – – – – 274* – –
Cavallo et al. 2024 3.21 1.63 – 316 -0.240 – – –
Hunt & Reffert 2023 3.45 1.50 0.43 138 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 1835 84.0 96.58 8.23 0.28 0.18 -1.76 46.5 0.11

💡 Note: The % column shows the percentage of members that Theia 2615 shares with each listed object.

Visualization

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