Theia 387

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0.59 UTI
0.75
CN
0.83
Cdens
0.75
CC3
0.31
Clit
1.0
Cdup
Radius (P>50% members) 32.3 [arcmin]
  • CN 0.75 Rich
  • Cdens 0.83 Dense
  • CC3 0.75 High quality
  • Clit 0.31 Poorly studied
  • Cdup 1.0 Unique

Overview

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Theia 387 is a rich, dense object of high C3 quality. Its parallax locates it at a close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is poorly studied in the literature.
Close Low extinction Near-solar metallicity Young

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 – 79.246 37.256 1.868 -0.556 -9.224 5.657
Zhang et al. 2024 79.153 37.199 – – – –
Hunt & Reffert 2024 79.153 37.199 1.848 -0.474 -9.146 5.615
Cavallo et al. 2024 79.251 37.278 1.853 – – –
Hunt & Reffert 2023 79.153 37.199 1.848 -0.474 -9.146 5.615
He et al. 2022 79.149 37.343 1.871 -0.55 -9.243 –

💡 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 – – – – -0.063* – – –
Hunt & Reffert 2024 – – – – – 109* – –
Cavallo et al. 2024 0.55 0.87 – 59 -0.080 – – –
Hunt & Reffert 2023 0.51 0.49 0.88 110 – – – –
He et al. 2022 – 0.85 – 63 – – – –

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

Visualization

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