Theia 19

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0.18 UTI
0.0
CN
1.0
Cdens
0.75
CC3
0.25
Clit
0.4
Cdup
Radius (P>50% members) 4.4 [arcmin]
  • CN 0.0 Sparse
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 0.4 Possibly duplicate

Overview

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Theia 19 is a sparse, very dense object of high C3 quality. Its parallax locates it at a close distance, above 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 possibly a duplicate object, which shares a significant percentage of members with at least one previously reported entry. See table with shared members information.

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 – 3.213 65.576 1.395 2.397 -2.431 -12.653
Hunt & Reffert 2024 3.221 65.566 1.387 2.423 -2.396 -12.631
Cavallo et al. 2024 3.389 65.673 1.381 – – –
Hunt & Reffert 2023 3.221 65.566 1.387 2.423 -2.396 -12.631
He et al. 2022 3.116 65.692 1.398 2.466 -2.387 –

💡 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 – – – – – 98* – –
Cavallo et al. 2024 0.99 2.12 – 2 0.290 – – –
Hunt & Reffert 2023 0.69 3.01 1.55 4 – – – –
He et al. 2022 – 1.90 – 2 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
OC 0223 60.0 3.2 65.56 1.39 2.38 -2.49 -12.38 0.4

💡 Note: The % column shows the percentage of members that Theia 19 shares with each listed object.

Visualization

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