CWNU 207

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0.23 UTI
0.0
CN
0.63
Cdens
0.5
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 10.9 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.63 Moderately dense
  • CC3 0.5 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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CWNU 207 is a sparse, moderately dense object of intermediate C3 quality. Its parallax locates it at a close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It is rarely studied in the literature.

âš ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Close Low extinction Near-solar metallicity Very young

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as a moving group.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 135.593 -46.834 1.201 -7.395 5.193 11.382
Cavallo et al. 2024 135.399 -46.77 1.198 – – –
Hunt & Reffert 2023 135.758 -46.863 1.183 -7.413 5.21 52.235
He et al. 2022 135.637 -46.855 1.2 -7.49 5.15 –

💡 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
Cavallo et al. 2024 0.96 0.87 – 3 -0.030 – – –
Hunt & Reffert 2023 0.80 0.81 1.49 4 – – – –
He et al. 2022 0.63 1.38 – 10 -0.930 – – –

Visualization

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