CWNU 1761

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0.52 UTI
0.35
CN
1.0
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 1.8 [arcmin]
  • CN 0.35 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 1761 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.
Relatively close High extinction 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 – 307.236 33.166 0.285 -1.326 -3.058 19.819
Hunt & Reffert 2024 307.233 33.164 0.298 -1.329 -3.037 24.993
Cavallo et al. 2024 307.216 33.169 0.295 – – –
Hunt & Reffert 2023 307.233 33.164 0.298 -1.329 -3.037 24.993
He et al. 2023 307.225 33.167 0.291 -1.307 -3.045 19.82

💡 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 – – – – – 251* – –
Cavallo et al. 2024 3.63 3.86 – 708 -0.030 – – –
Hunt & Reffert 2023 2.97 4.22 2.33 526 – – – –
He et al. 2023 2.82 4.05 – 708 – – – –

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

Visualization

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