Theia 7490

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0.16 UTI
0.27
CN
0.18
Cdens
0.38
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 9.7 [arcmin]
  • CN 0.27 Poorly populated
  • Cdens 0.18 Very loose
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
Theia 7490 is a poorly populated, very loose object of low C3 quality. Its parallax locates it at a relatively close distance, near 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: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Relatively close 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 – 183.503 -63.784 0.513 -8.036 -0.513 -9.731
Hunt & Reffert 2024 183.352 -63.757 0.521 -8.032 -0.547 -9.47
Cavallo et al. 2024 184.121 -63.852 0.524 – – –
Hunt & Reffert 2023 183.352 -63.757 0.521 -8.032 -0.547 -9.47

💡 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 – – – – – 57* – –
Cavallo et al. 2024 1.41 1.22 – 186 -0.420 – – –
Hunt & Reffert 2023 1.82 0.91 0.58 202 – – – –

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

Visualization

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