CWNU 2541

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0.36 UTI
0.42
CN
0.61
Cdens
0.25
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 3.9 [arcmin]
  • CN 0.42 Poorly populated
  • Cdens 0.61 Moderately dense
  • CC3 0.25 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 2541 is a poorly populated, moderately dense object of low C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It was recently reported in the literature.
Distant Moderate 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 – 334.534 53.731 0.306 -4.097 -4.187 -65.98
Hunt & Reffert 2024 334.537 53.721 0.305 -4.088 -4.169 -65.991
Cavallo et al. 2024 334.623 53.812 0.305 – – –
Hunt & Reffert 2023 334.537 53.721 0.305 -4.088 -4.169 -65.991
He et al. 2023 334.511 53.746 0.322 -4.111 -4.18 -65.98

💡 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 – – – – – 213* – –
Cavallo et al. 2024 3.12 2.07 – 51 -0.090 – – –
Hunt & Reffert 2023 3.01 1.26 2.43 78 – – – –
He et al. 2023 2.82 2.00 – 447 – – – –

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

Visualization

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