Theia 15

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0.02 UTI
0.0
CN
1.0
Cdens
1.0
CC3
0.25
Clit
0.04
Cdup
Radius (P>50% members) 3.8 [arcmin]
  • CN 0.0 Sparse
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.25 Poorly studied
  • Cdup 0.04 Very likely duplicate

Overview

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Theia 15 is a sparse, very dense object of very high C3 quality. Its parallax locates it at a close distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It is poorly studied 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.

Relatively close Moderate extinction Near-solar metallicity Very young

Cavallo et al. (2024)
Bronze sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 90.868 -9.746 1.177 -2.237 1.619 46.287
Hunt & Reffert 2024 90.882 -9.742 1.187 -2.145 1.551 37.499
Cavallo et al. 2024 90.895 -9.784 1.181 – – –
Hunt & Reffert 2023 90.882 -9.742 1.187 -2.145 1.551 37.499
He et al. 2022 90.779 -9.798 1.205 -1.954 1.718 –

💡 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 – – – – – 62* – –
Cavallo et al. 2024 1.24 1.75 – 8 -0.110 – – –
Hunt & Reffert 2023 0.80 1.35 1.54 6 – – – –
He et al. 2022 – 0.05 – 3 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
OC 0362 96.0 90.89 -9.79 1.19 -2.11 1.64 39.52 0.47
CWWDL 14261 64.0 90.89 -9.75 1.16 -2.05 1.62 44.56 0.01
OC 0361 52.0 90.56 -9.92 1.23 -2.02 1.77 18.13 0.35

💡 Note: The % column shows the percentage of members that Theia 15 shares with each listed object.

Visualization

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