CWNU 1553

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0.39 UTI
0.28
CN
0.44
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 3.3 [arcmin]
  • CN 0.28 Poorly populated
  • Cdens 0.44 Loose
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 1553 is a poorly populated, loose 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 metal-rich, young cluster (see Parameters). It was recently reported in the literature.
Distant High extinction Metal-rich Young

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 – 151.672 -55.449 0.27 -5.859 3.804 –
Hunt & Reffert 2024 151.665 -55.439 0.255 -5.851 3.808 –
Cavallo et al. 2024 151.706 -55.441 0.258 – – –
Hunt & Reffert 2023 151.665 -55.439 0.255 -5.851 3.808 –
He et al. 2023 151.669 -55.445 0.27 -5.911 3.799 –

💡 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 – – – – – 431* – –
Cavallo et al. 2024 3.34 3.58 – 37 0.550 – – –
Hunt & Reffert 2023 3.32 3.90 2.12 20 – – – –
He et al. 2023 3.24 4.15 – 7 – – – –

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

Visualization

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