Theia 2819

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0.06 UTI
0.52
CN
1.0
Cdens
0.75
CC3
0.0
Clit
0.13
Cdup
Radius (P>50% members) 3.7 [arcmin]
  • CN 0.52 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 0.13 Likely duplicate

Overview

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Theia 2819 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate 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.

Relatively close Moderate 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 – 214.656 -62.659 0.46 -3.896 -2.535 -4.997
Hunt & Reffert 2024 214.683 -62.665 0.457 -3.91 -2.55 –
Cavallo et al. 2024 214.601 -62.643 0.457 – – –
Hunt & Reffert 2023 214.683 -62.665 0.457 -3.91 -2.55 –

💡 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 – – – – – 389* – –
Cavallo et al. 2024 2.02 1.77 – 209 0.490 – – –
Hunt & Reffert 2023 2.00 2.07 2.23 37 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
UFMG 60 87.3 214.67 -62.66 0.46 -3.88 -2.53 -5.0 0.5
LISC 3170 74.5 214.65 -62.66 0.46 -3.91 -2.55 – 0.07

💡 Note: The % column shows the percentage of members that Theia 2819 shares with each listed object.

Visualization

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