CWNU 1353

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0.54 UTI
0.44
CN
1.0
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 2.5 [arcmin]
  • CN 0.44 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 1353 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a moderate 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 – 207.766 -62.289 0.319 -7.261 -1.692 -51.795
Hunt & Reffert 2024 207.741 -62.289 0.323 -7.225 -1.694 -51.823
Cavallo et al. 2024 207.764 -62.281 0.322 – – –
Hunt & Reffert 2023 207.741 -62.289 0.323 -7.225 -1.694 -51.823
He et al. 2023 207.756 -62.292 0.33 -7.262 -1.696 -49.86

💡 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 – – – – – 447* – –
Cavallo et al. 2024 2.86 3.10 – 240 0.160 – – –
Hunt & Reffert 2023 2.90 3.41 1.62 79 – – – –
He et al. 2023 2.69 3.55 – 158 – – – –

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

Visualization

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