Theia 7778

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0.30 UTI
0.0
CN
0.25
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 5.8 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.25 Loose
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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Theia 7778 is a sparse, loose object of high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by low extinction. It is catalogued as a low-mass, 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.
Relatively close Low extinction Low mass 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 – 311.726 35.708 0.444 -2.904 -4.218 –
Zhang et al. 2024 311.802 35.635 – – – –
Hunt & Reffert 2024 311.802 35.635 0.43 -2.859 -4.224 –
Cavallo et al. 2024 311.723 35.757 0.431 – – –
Hunt & Reffert 2023 311.802 35.635 0.43 -2.859 -4.224 –

💡 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 – – – – -0.310* – – –
Hunt & Reffert 2024 – – – – – 44* – –
Cavallo et al. 2024 2.29 0.93 – 123 0.200 – – –
Hunt & Reffert 2023 2.10 0.81 0.65 219 – – – –

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

Visualization

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