Theia 1761

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0.06 UTI
0.54
CN
0.93
Cdens
1.0
CC3
0.0
Clit
0.12
Cdup
Radius (P>50% members) 8.5 [arcmin]
  • CN 0.54 Moderately populated
  • Cdens 0.93 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.0 Rarely studied
  • Cdup 0.12 Likely duplicate

Overview

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Theia 1761 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a relatively close distance, near 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.

Relatively close Moderate extinction Metal-poor 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 – 268.605 -23.086 0.706 0.08 -2.609 -5.403
Hunt & Reffert 2024 268.602 -23.109 0.702 0.089 -2.591 -7.219
Cavallo et al. 2024 268.594 -23.06 0.707 – – –
Hunt & Reffert 2023 268.602 -23.109 0.702 0.089 -2.591 -7.219

💡 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 – – – – – 976* – –
Cavallo et al. 2024 1.08 3.05 – 13 -0.820 – – –
Hunt & Reffert 2023 1.33 2.54 2.24 43 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWWDL 14199 87.7 268.6 -23.09 0.71 0.08 -2.61 0.14 0.14
UFMG 72 71.9 268.53 -23.13 0.71 0.08 -2.61 -10.55 0.48

💡 Note: The % column shows the percentage of members that Theia 1761 shares with each listed object.

Visualization

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