CWNU 1398

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0.33 UTI
0.0
CN
0.88
Cdens
0.25
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 4.4 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.88 Dense
  • CC3 0.25 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 1398 is a sparse, dense object of low C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, 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 P198, along with FoF_1182.

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 99999– 237.365 -55.94 0.509 -0.846 -2.709 –
Hunt & Reffert 2024 237.373 -55.93 0.505 -0.839 -2.727 –
Cavallo et al. 2024 237.381 -55.967 0.502 – – –
Hunt & Reffert 2023 237.373 -55.93 0.505 -0.839 -2.727 –
He et al. 2023 237.364 -55.942 0.518 -0.853 -2.691 –

💡 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– 2.0 3.8 1.99 48 -0.400 238 – –
Hunt & Reffert 2024 – – – – – 238(1) – –
Cavallo et al. 2024 2.10 4.03 – 48 -0.400 – – –
Hunt & Reffert 2023 1.87 3.59 1.99 200 – – – –
He et al. 2023 2.00 3.80 – 6 – – – –

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

Visualization

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