CWNU 2415

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0.63 UTI
0.63
CN
1.0
Cdens
1.0
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 1.3 [arcmin]
  • CN 0.63 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 2415 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a large* distance, above the mid-plane, affected by high extinction. It is catalogued as a massive, near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.

(*): The parallax distance estimate (~6.70 kpc) differs significantly from the median photometric distance (~4.85 kpc).

Distant High extinction Massive Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Silver sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 298.379 29.868 0.149 -2.75 -5.275 -5.371
Hunt & Reffert 2024 298.379 29.869 0.142 -2.734 -5.273 -0.965
Cavallo et al. 2024 298.38 29.871 0.143 – – –
Hunt & Reffert 2023 298.379 29.869 0.142 -2.734 -5.273 -0.965
He et al. 2023 298.38 29.874 0.173 -2.76 -5.29 -5.37

💡 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 – – – – – 2982* – –
Cavallo et al. 2024 4.85 4.45 – 263 -0.450 – – –
Hunt & Reffert 2023 5.66 3.53 2.77 596 – – – –
He et al. 2023 4.27 3.85 – 562 – – – –

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

Visualization

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