Theia 1797

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0.09 UTI
0.27
CN
0.29
Cdens
0.38
CC3
0.25
Clit
0.3
Cdup
Radius (P>50% members) 12.4 [arcmin]
  • CN 0.27 Poorly populated
  • Cdens 0.29 Loose
  • CC3 0.38 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 0.3 Possibly duplicate

Overview

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Theia 1797 is a poorly populated, 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, very young 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 Moderate extinction Near-solar metallicity Very 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 – 99.067 9.929 0.843 -1.577 -0.909 16.049
Zhang et al. 2024 99.071 9.833 – – – –
Hunt & Reffert 2024 99.071 9.833 0.866 -1.582 -0.93 20.151
Cavallo et al. 2024 99.045 10.028 0.867 – – –
Hunt & Reffert 2023 99.071 9.833 0.866 -1.582 -0.93 20.151

💡 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 – – – – -0.072* – – –
Hunt & Reffert 2024 – – – – – 325* – –
Cavallo et al. 2024 1.20 1.29 – 10 -0.050 – – –
Hunt & Reffert 2023 1.07 1.14 2.20 28 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 1208 70.4 99.07 9.95 0.84 -1.58 -0.87 16.05 0.06
CWNU 81 40.7 98.96 10.24 0.85 -1.61 -0.88 5.04 0.11

💡 Note: The % column shows the percentage of members that Theia 1797 shares with each listed object.

Visualization

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