CWNU 1648

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0.50 UTI
0.26
CN
1.0
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 2.7 [arcmin]
  • CN 0.26 Poorly populated
  • 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 1648 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It was recently reported in the literature.
Relatively close Moderate extinction Near-solar metallicity 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 – 245.216 -49.91 0.36 -0.943 -1.683 -40.5
Hunt & Reffert 2024 245.24 -49.905 0.36 -0.96 -1.677 -40.94
Cavallo et al. 2024 245.216 -49.903 0.359 – – –
Hunt & Reffert 2023 245.24 -49.905 0.36 -0.96 -1.677 -40.94
He et al. 2023 245.225 -49.914 0.362 -0.945 -1.671 -50.32

💡 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 – – – – – 403* – –
Cavallo et al. 2024 2.28 2.67 – 126 0.290 – – –
Hunt & Reffert 2023 2.57 2.61 1.77 99 – – – –
He et al. 2023 2.63 2.80 – 4 – – – –

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

Visualization

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