Theia 96

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0.00 UTI
0.76
CN
1.0
Cdens
1.0
CC3
0.25
Clit
0.0
Cdup
Radius (P>50% members) 39.2 [arcmin]
  • CN 0.76 Rich
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.25 Poorly studied
  • Cdup 0.0 Very likely duplicate

Overview

â„šī¸
Theia 96 is a rich, very dense object of very high C3 quality. Its parallax locates it at a very close distance, above the mid-plane, affected by low 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 very 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 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 – 305.279 48.772 2.841 3.002 1.965 -7.956
Zhang et al. 2024 305.287 48.925 – – – –
Hunt & Reffert 2024 305.287 48.925 2.846 3.03 1.965 -12.675
Cavallo et al. 2024 305.134 48.881 2.843 – – –
Hunt & Reffert 2023 305.287 48.925 2.846 3.03 1.965 -12.675

💡 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 – – – – 0.052* – – –
Hunt & Reffert 2024 – – – – – 73* – –
Cavallo et al. 2024 0.36 0.61 – 17 0.000 – – –
Hunt & Reffert 2023 0.35 0.15 0.62 22 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
OCSN 23 100.0 305.13 48.62 2.86 3.16 1.97 -7.7 0.52
LISC-III 3723 64.3 304.16 46.65 2.92 3.51 1.72 -7.45 0.27

💡 Note: The % column shows the percentage of members that Theia 96 shares with each listed object.

Visualization

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