CWNU 407

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0.54 UTI
0.54
CN
0.89
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 5.7 [arcmin]
  • CN 0.54 Moderately populated
  • Cdens 0.89 Dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 407 is a moderately populated, 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, near-solar metallicity, young cluster (see Parameters). It is poorly studied in the literature.
Relatively close High extinction Massive 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 – 279.516 -6.443 0.464 0.046 -0.511 27.698
Hunt & Reffert 2024 279.497 -6.466 0.461 0.042 -0.532 33.615
Cavallo et al. 2024 279.576 -6.367 0.46 – – –
Hunt & Reffert 2023 279.497 -6.466 0.461 0.042 -0.532 33.615
He et al. 2022 279.546 -6.383 0.48 0.07 -0.54 –

💡 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 – – – – – 1068* – –
Cavallo et al. 2024 2.34 4.08 – 89 0.130 – – –
Hunt & Reffert 2023 2.01 3.75 2.55 69 – – – –
He et al. 2022 1.86 3.54 – 398 -0.082 – – –

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

Visualization

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