CWNU 1536

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0.51 UTI
0.28
CN
1.0
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 1.7 [arcmin]
  • CN 0.28 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 1536 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It was recently reported in the literature.
Distant High extinction Near-solar metallicity 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 – 212.393 -61.703 0.269 -6.02 -1.731 -75.865
Hunt & Reffert 2024 212.388 -61.7 0.268 -6.034 -1.72 -75.875
Cavallo et al. 2024 212.387 -61.707 0.269 – – –
Hunt & Reffert 2023 212.388 -61.7 0.268 -6.034 -1.72 -75.875
He et al. 2023 212.386 -61.705 0.268 -6.024 -1.747 –

💡 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 – – – – – 461* – –
Cavallo et al. 2024 3.25 3.70 – 11 0.120 – – –
Hunt & Reffert 2023 3.55 3.84 2.49 17 – – – –
He et al. 2023 4.27 4.25 – 4 – – – –

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

Visualization

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