CWNU 2848

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0.35 UTI
0.0
CN
1.0
Cdens
0.25
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 9.2 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 1.0 Very dense
  • CC3 0.25 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 2848 is a sparse, very dense object of low C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age 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 P363, along with CWNU_2719.

Cavallo et al. (2024)
Silver 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– 274.076 -19.387 0.505 0.455 -1.882 –
Hunt & Reffert 2024 274.082 -19.394 0.501 0.457 -1.88 –
Cavallo et al. 2024 274.086 -19.379 0.501 – – –
Hunt & Reffert 2023 274.082 -19.394 0.501 0.457 -1.88 –
He et al. 2023 274.08 -19.393 0.505 0.47 -1.878 –

💡 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– 1.86 1.6 1.91 104 0.230 130 – –
Hunt & Reffert 2024 – – – – – 130(1) – –
Cavallo et al. 2024 1.48 1.60 – 457 0.230 – – –
Hunt & Reffert 2023 1.88 1.73 1.91 104 – – – –
He et al. 2023 1.86 1.60 – 5 – – – –

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

Visualization

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