CWNU 1556

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0.55 UTI
0.25
CN
1.0
Cdens
1.0
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 6.5 [N/pc2]
  • CN 0.25 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 1556 is a poorly populated, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by very high extinction. It is catalogued as a near-solar metallicity, very young cluster, but with a large variance across recent sources for the age parameter (see Parameters). It was recently reported in the literature.

Cavallo et al. (2024)
Wood 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– 290.244 13.3 0.237 -2.75 -5.695 4.879
Hunt & Reffert 2024 290.241 13.3 0.244 -2.735 -5.682 26.309
Cavallo et al. 2024 290.272 13.31 0.243 – – –
Hunt & Reffert 2023 290.241 13.3 0.244 -2.735 -5.682 26.309
He et al. 2023 290.247 13.295 0.25 -2.748 -5.687 –

💡 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– 3.47 6.16 2.81 4 0.300 612 – –
Hunt & Reffert 2024 – – – – – 612(1) – –
Cavallo et al. 2024 3.10 5.57 – 4 0.300 – – –
Hunt & Reffert 2023 3.76 6.16 2.81 61 – – – –
He et al. 2023 3.47 8.10 – 1 – – – –

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

Visualization

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