CWNU 1500

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0.45 UTI
0.0
CN
1.0
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 25.7 [N/pc2]
  • CN 0.0 Sparse
  • 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 1500 is a sparse, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by high extinction. It is catalogued as a metal-rich, very young cluster, but with a large variance across recent sources for the age parameter (see Parameters). It was recently reported in the literature.

Palma et al. (2025)
Classified as optical pair P313, along with CWNU_2088.

Cavallo et al. (2024)
Bronze sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 194.341 -61.392 0.554 -6.56 -2.152 -7.626
Hunt & Reffert 2024 194.325 -61.394 0.55 -6.573 -2.14 -9.024
Cavallo et al. 2024 194.269 -61.394 0.55 – – –
Hunt & Reffert 2023 194.325 -61.394 0.55 -6.573 -2.14 -9.024
He et al. 2023 194.338 -61.394 0.559 -6.56 -2.163 –

💡 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] Bfrac BSS
UCC 99999– 1.73 4.14 1.48 7 0.620 328 – –
Hunt & Reffert 2024 – – – – – 328(1) – –
Cavallo et al. 2024 1.74 3.28 – 54 0.620 – – –
Hunt & Reffert 2023 1.73 4.14 1.48 7 – – – –
He et al. 2023 1.70 4.40 – 6 – – – –

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Visualization

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