CWNU 1760

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0.27 UTI
0.0
CN
0.61
Cdens
0.12
CC3
0.31
Clit
1.0
Cdup
Radius (P>50% members) 4.9 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.61 Moderately dense
  • CC3 0.12 Very low quality
  • Clit 0.31 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 1760 is a sparse, moderately dense object of very low C3 quality. Its parallax locates it at a relatively close distance, near 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 – 66.465 48.735 0.509 0.168 -2.391 90.298
Zhang et al. 2024 66.482 48.762 – – – –
Hunt & Reffert 2024 66.482 48.762 0.517 0.132 -2.359 115.844
Cavallo et al. 2024 66.478 48.725 0.516 – – –
Hunt & Reffert 2023 66.482 48.762 0.517 0.132 -2.359 115.844
He et al. 2023 66.465 48.743 0.518 0.168 -2.395 -28.06

💡 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
Zhang et al. 2024 – – – – 0.081* – – –
Hunt & Reffert 2024 – – – – – 154* – –
Cavallo et al. 2024 2.84 3.97 – 66 0.040 – – –
Hunt & Reffert 2023 1.85 3.55 2.27 196 – – – –
He et al. 2023 2.04 4.15 – 447 – – – –

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

Visualization

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