CWNU 2405

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0.42 UTI
0.33
CN
0.53
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 4.9 [arcmin]
  • CN 0.33 Poorly populated
  • Cdens 0.53 Moderately dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 2405 is a poorly populated, moderately dense object of high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It was recently reported in the literature.
Relatively close Low 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 – 185.13 -65.633 0.406 -5.335 -0.507 –
Hunt & Reffert 2024 185.081 -65.637 0.409 -5.296 -0.51 –
Cavallo et al. 2024 185.248 -65.57 0.407 – – –
Hunt & Reffert 2023 185.081 -65.637 0.409 -5.296 -0.51 –
He et al. 2023 185.145 -65.616 0.411 -5.312 -0.52 –

💡 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 – – – – – 137* – –
Cavallo et al. 2024 2.04 0.68 – 22 -0.250 – – –
Hunt & Reffert 2023 2.26 0.60 1.10 39 – – – –
He et al. 2023 2.51 1.05 – 9 – – – –

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

Visualization

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