Theia 1975

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0.06 UTI
0.0
CN
0.18
Cdens
0.38
CC3
0.0
Clit
0.52
Cdup
Radius (P>50% members) 8.5 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.18 Very loose
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 0.52 Likely unique

Overview

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Theia 1975 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a massive, metal-rich, very young cluster (see Parameters). It was recently reported in the literature.

Note: This is likely a unique object, which shares a moderate percentage of members with at least one previously reported entry. See table with shared members information.

Relatively close High extinction Massive Metal-rich Very 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 – 305.517 37.039 0.495 -2.402 -5.356 53.948
Hunt & Reffert 2024 305.387 36.932 0.497 -2.424 -5.347 21.699
Cavallo et al. 2024 305.61 37.152 0.495 – – –
Hunt & Reffert 2023 305.387 36.932 0.497 -2.424 -5.347 21.699

💡 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 – – – – – 1053* – –
Cavallo et al. 2024 2.23 3.74 – 13 0.810 – – –
Hunt & Reffert 2023 1.96 4.08 2.76 7 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWWDL 1872 48.0 305.53 37.13 0.5 -2.43 -5.33 53.95 0.05
UBC 1101 44.0 305.72 37.19 0.49 -2.38 -5.32 46.61 0.44
XDOCC 10 20.0 305.52 37.24 0.5 -2.4 -5.26 53.95 0.25
UBC 1098 16.0 305.39 36.93 0.49 -2.63 -5.41 -134.78 0.38

💡 Note: The % column shows the percentage of members that Theia 1975 shares with each listed object.

Visualization

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