Theia 2449

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0.08 UTI
0.3
CN
0.17
Cdens
0.12
CC3
0.25
Clit
0.37
Cdup
Radius (P>50% members) 17.8 [arcmin]
  • CN 0.3 Poorly populated
  • Cdens 0.17 Very loose
  • CC3 0.12 Very low quality
  • Clit 0.25 Poorly studied
  • Cdup 0.37 Possibly duplicate

Overview

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Theia 2449 is a poorly populated, very loose object of very low C3 quality. Its parallax locates it at a relatively close distance, near 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.

âš ī¸ Warning: This is possibly a duplicate object, which shares a significant percentage of members with at least one previously reported entry. See table with shared members information.

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 – 102.378 -3.724 0.86 -0.078 -0.925 -0.821
Zhang et al. 2024 102.355 -3.731 – – – –
Hunt & Reffert 2024 102.355 -3.731 0.868 -0.057 -0.997 -1.541
Cavallo et al. 2024 102.187 -3.742 0.872 – – –
Hunt & Reffert 2023 102.355 -3.731 0.868 -0.057 -0.997 -1.541

💡 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 – – – – – 65* – –
Cavallo et al. 2024 1.11 0.67 – 417 -0.150 – – –
Hunt & Reffert 2023 1.07 0.67 0.51 275 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 1041 63.3 102.43 -3.71 0.85 -0.14 -0.84 -8.19 0.07

💡 Note: The % column shows the percentage of members that Theia 2449 shares with each listed object.

Visualization

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