CWNU 1630

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0.46 UTI
0.31
CN
0.73
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 7.3 [arcmin]
  • CN 0.31 Poorly populated
  • Cdens 0.73 Moderately dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 1630 is a poorly populated, moderately dense object of high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, very young cluster, but with a large variance across recent sources for the age parameter (see Parameters). It was recently reported in the literature.
Relatively close Low extinction Near-solar metallicity Very 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 – 273.722 -20.439 0.727 1.48 -1.198 12.933
Hunt & Reffert 2024 273.733 -20.415 0.728 1.5 -1.166 7.603
Cavallo et al. 2024 273.695 -20.417 0.728 – – –
Hunt & Reffert 2023 273.733 -20.415 0.728 1.5 -1.166 7.603
He et al. 2023 273.702 -20.475 0.731 1.481 -1.199 –

💡 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 – – – – – 223* – –
Cavallo et al. 2024 1.47 0.85 – 63 -0.210 – – –
Hunt & Reffert 2023 1.28 0.87 1.22 9 – – – –
He et al. 2023 1.32 1.25 – 8 – – – –

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

Visualization

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