Theia 2561

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0.15 UTI
0.58
CN
1.0
Cdens
0.75
CC3
0.0
Clit
0.31
Cdup
Radius (P>50% members) 9.5 [arcmin]
  • CN 0.58 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 0.31 Possibly duplicate

Overview

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Theia 2561 is a moderately populated, very dense object of 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 near-solar metallicity, young cluster (see Parameters). It was recently reported 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.

Relatively close Moderate extinction Near-solar metallicity 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 – 318.459 46.382 0.797 -2.965 -3.507 12.289
Hunt & Reffert 2024 318.48 46.407 0.801 -2.962 -3.511 10.061
Cavallo et al. 2024 318.503 46.384 0.799 – – –
Hunt & Reffert 2023 318.48 46.407 0.801 -2.962 -3.511 10.061

💡 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 – – – – – 349* – –
Cavallo et al. 2024 1.26 1.41 – 46 0.050 – – –
Hunt & Reffert 2023 1.20 1.13 2.25 59 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWWDL 13502 68.7 318.54 46.38 0.8 -2.97 -3.51 12.29 0.11
UBC 1129 56.7 318.51 46.38 0.79 -2.97 -3.5 2.66 0.38
CWNU 1249 38.8 318.44 46.39 0.8 -2.96 -3.54 19.93 0.06

💡 Note: The % column shows the percentage of members that Theia 2561 shares with each listed object.

Visualization

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