Theia 2782

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0.25 UTI
0.0
CN
0.1
Cdens
0.62
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 14.5 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.1 Very loose
  • CC3 0.62 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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Theia 2782 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.
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 – 102.912 9.244 0.665 -2.431 -0.042 –
Zhang et al. 2024 102.971 9.236 – – – –
Hunt & Reffert 2024 102.971 9.236 0.663 -2.431 -0.074 –
Cavallo et al. 2024 102.953 9.371 0.665 – – –
Hunt & Reffert 2023 102.971 9.236 0.663 -2.431 -0.074 –

💡 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 – – – – -0.219* – – –
Hunt & Reffert 2024 – – – – – 131* – –
Cavallo et al. 2024 1.64 0.84 – 32 -0.020 – – –
Hunt & Reffert 2023 1.40 0.53 0.75 191 – – – –

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

Visualization

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