CWNU 2560

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0.60 UTI
0.76
CN
1.0
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 2.9 [arcmin]
  • CN 0.76 Rich
  • 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 2560 is a rich, very dense object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a massive, metal-rich, young cluster (see Parameters). It was recently reported in the literature.
Relatively close High extinction Massive Metal-rich Young

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 – 253.204 -46.369 0.403 -2.736 -4.194 -16.407
Hunt & Reffert 2024 253.207 -46.365 0.403 -2.73 -4.178 1.702
Cavallo et al. 2024 253.202 -46.378 0.398 – – –
Hunt & Reffert 2023 253.207 -46.365 0.403 -2.73 -4.178 1.702
He et al. 2023 253.21 -46.372 0.414 -2.739 -4.211 19.28

💡 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] Bfr BSS
Hunt & Reffert 2024 – – – – – 3856* – –
Cavallo et al. 2024 2.92 4.42 – 66 0.830 – – –
Hunt & Reffert 2023 2.28 4.79 2.96 103 – – – –
He et al. 2023 2.19 5.25 – 79 – – – –

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Visualization

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