CWNU 1516

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0.16 UTI
0.0
CN
0.06
Cdens
0.12
CC3
0.31
Clit
1.0
Cdup
Radius (P>50% members) 8.4 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.06 Very loose
  • CC3 0.12 Very low quality
  • Clit 0.31 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 1516 is a sparse, very loose object of very 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.
Distant Moderate extinction Near-solar metallicity Intermediate age

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 – 96.598 4.469 0.301 0.091 -1.083 55.486
Zhang et al. 2024 96.637 4.506 – – – –
Hunt & Reffert 2024 96.637 4.506 0.289 0.089 -1.044 55.5
Cavallo et al. 2024 96.602 4.444 0.291 – – –
Hunt & Reffert 2023 96.637 4.506 0.289 0.089 -1.044 55.5
He et al. 2023 96.595 4.427 0.288 0.11 -1.089 36.06

💡 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 – – – – -0.214* – – –
Hunt & Reffert 2024 – – – – – 125* – –
Cavallo et al. 2024 2.73 2.13 – 324 0.110 – – –
Hunt & Reffert 2023 3.03 1.91 1.36 210 – – – –
He et al. 2023 3.02 2.20 – 316 – – – –

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

Visualization

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