CWNU 1478

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0.60 UTI
0.5
CN
1.0
Cdens
1.0
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 2.4 [arcmin]
  • CN 0.5 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 1478 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by very high extinction. It is catalogued as a massive, near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.
Distant Very high extinction Massive Near-solar metallicity Intermediate age

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 – 214.969 -61.931 0.28 -5.149 -3.381 -31.413
Hunt & Reffert 2024 214.969 -61.945 0.286 -5.144 -3.367 -14.03
Cavallo et al. 2024 214.971 -61.932 0.292 – – –
Hunt & Reffert 2023 214.969 -61.945 0.286 -5.144 -3.367 -14.03
He et al. 2023 214.954 -61.935 0.319 -5.148 -3.382 -33.18

💡 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 – – – – – 1209* – –
Cavallo et al. 2024 2.54 4.90 – 257 -0.060 – – –
Hunt & Reffert 2023 3.05 5.12 2.62 119 – – – –
He et al. 2023 3.63 5.35 – 112 – – – –

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

Visualization

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