CWNU 304

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0.49 UTI
0.52
CN
0.42
Cdens
1.0
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 8.8 [arcmin]
  • CN 0.52 Moderately populated
  • Cdens 0.42 Loose
  • CC3 1.0 Very high quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 304 is a moderately populated, loose object of very high C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is poorly studied in the literature.
Relatively close Moderate extinction 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 – 251.085 -53.148 0.51 -2.067 -3.757 -23.94
Hunt & Reffert 2024 251.129 -52.988 0.505 -2.063 -3.751 -22.219
Cavallo et al. 2024 251.112 -53.132 0.505 – – –
Hunt & Reffert 2023 251.129 -52.988 0.505 -2.063 -3.751 -22.219
He et al. 2022 251.051 -53.202 0.51 -2.08 -3.75 -27.6

💡 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 – – – – – 235* – –
Cavallo et al. 2024 1.91 1.31 – 372 0.340 – – –
Hunt & Reffert 2023 1.85 1.06 0.67 372 – – – –
He et al. 2022 1.48 1.50 – 501 -1.335 – – –

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

Visualization

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