Theia 517

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0.07 UTI
0.84
CN
1.0
Cdens
1.0
CC3
0.25
Clit
0.1
Cdup
Radius (P>50% members) 54.8 [arcmin]
  • CN 0.84 Rich
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.25 Poorly studied
  • Cdup 0.1 Likely duplicate

Overview

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Theia 517 is a rich, very dense object of very high C3 quality. Its parallax locates it at a very 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 likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

Very 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 – 322.799 48.253 3.364 -7.45 -19.738 -6.067
Zhang et al. 2024 322.83 48.349 – – – –
Hunt & Reffert 2024 322.831 48.349 3.366 -7.4 -19.704 -5.362
Cavallo et al. 2024 322.65 48.189 3.367 – – –
Hunt & Reffert 2023 322.831 48.349 3.366 -7.4 -19.704 -5.362

💡 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 – – – – -0.088* – – –
Hunt & Reffert 2024 – – – – – 269* – –
Cavallo et al. 2024 0.30 0.41 – 102 0.070 – – –
Hunt & Reffert 2023 0.29 0.07 0.38 126 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
Melotte 236 89.9 322.8 48.25 3.36 -7.45 -19.73 -5.94 0.97
CWWDL 14690 15.5 322.87 48.25 3.4 -7.49 -19.96 -6.46 0.0
CWWDL 14621 12.9 323.03 48.3 3.38 -7.6 -19.9 -6.53 0.0

💡 Note: The % column shows the percentage of members that Theia 517 shares with each listed object.

Visualization

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