CWNU 1317

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0.30 UTI
0.25
CN
0.39
Cdens
0.25
CC3
0.31
Clit
1.0
Cdup
Radius (P>50% members) 4.6 [arcmin]
  • CN 0.25 Poorly populated
  • Cdens 0.39 Loose
  • CC3 0.25 Low quality
  • Clit 0.31 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 1317 is a poorly populated, loose 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, intermediate-age cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It was recently reported in the literature.
Relatively close Moderate 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 – 70.516 33.058 0.373 1.432 -1.763 -3.337
Zhang et al. 2024 70.511 33.053 – – – –
Hunt & Reffert 2024 70.511 33.053 0.386 1.388 -1.728 -7.672
Cavallo et al. 2024 70.533 33.05 0.385 – – –
Hunt & Reffert 2023 70.511 33.053 0.386 1.388 -1.728 -7.672
He et al. 2023 70.512 33.06 0.382 1.392 -1.795 -0.93

💡 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 – – – – 0.197* – – –
Hunt & Reffert 2024 – – – – – 190* – –
Cavallo et al. 2024 2.77 2.76 – 245 -0.160 – – –
Hunt & Reffert 2023 2.36 2.34 0.91 714 – – – –
He et al. 2023 2.95 2.60 – 1413 – – – –

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

Visualization

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