Theia 2803

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0.10 UTI
0.37
CN
1.0
Cdens
1.0
CC3
0.0
Clit
0.22
Cdup
Stellar density (N50/rad) 7.7 [N/pc2]
  • CN 0.37 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.0 Rarely studied
  • Cdup 0.22 Likely duplicate

Overview

â„šī¸
Theia 2803 is a poorly populated, very dense object of very high C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a metal-poor, young 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.

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 99999– 263.156 -30.871 0.638 -0.748 -2.713 –
Hunt & Reffert 2024 263.153 -30.855 0.618 -0.754 -2.679 –
Cavallo et al. 2024 263.147 -30.855 0.618 – – –
Hunt & Reffert 2023 263.153 -30.855 0.618 -0.754 -2.679 –

💡 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] Bfrac BSS
UCC 99999– 1.355 2.925 1.23 38 -0.830 473 – –
Hunt & Reffert 2024 – – – – – 473(1) – –
Cavallo et al. 2024 1.21 3.27 – 46 -0.830 – – –
Hunt & Reffert 2023 1.50 2.58 1.23 29 – – – –

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
UFMG 68 78.4 263.14 -30.86 0.64 -0.7 -2.68 – 0.42

💡 Note: The % column shows the percentage of members that Theia 2803 shares with each listed object.

Visualization

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