CWNU 1488

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0.11 UTI
0.0
CN
0.06
Cdens
0.38
CC3
0.06
Clit
1.0
Cdup
Core radius and density 3.9 [pc], 0.3 [pc-2]
  • CN 0.0 Sparse
  • Cdens 0.06 Very loose
  • CC3 0.38 Low quality
  • Clit 0.06 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
CWNU 1488 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate distance, near 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.

âš ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Cavallo et al. (2024)
Bronze sample.

Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.20 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.20 (50th percentile).

Data

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 228.048 -57.396 0.365 -3.967 -3.495 -16.054
Hunt & Reffert 2024 228.054 -57.357 0.342 -4.054 -3.389 –
Cavallo et al. 2024 228.071 -57.383 0.345 – – –
Hunt & Reffert 2023 228.054 -57.357 0.342 -4.054 -3.389 –
He et al. 2023 228.03 -57.408 0.368 -3.948 -3.487 –

💡 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– 2.61 4.44 2.46 18 0.720 592 – –
Hunt & Reffert 2024 2.61 4.48 2.46 18 – 592(1) – –
Cavallo et al. 2024 2.78 4.19 – 29 0.720 – – –
Hunt & Reffert 2023 2.61 4.48 2.46 18 – – – –
He et al. 2023 2.45 4.40 – 4 – – – –

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

Visualization

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