CWNU 1998

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0.40 UTI
0.0
CN
0.5
Cdens
1.0
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 6.3 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.5 Moderately dense
  • CC3 1.0 Very high quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 1998 is a sparse, moderately dense object of very high C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by moderate extinction. It is catalogued as a metal-poor, intermediate-age cluster (see Parameters). It was recently reported in the literature.
Relatively close Moderate extinction Metal-poor 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 – 267.477 -33.376 0.635 0.035 -1.986 –
Hunt & Reffert 2024 267.466 -33.335 0.639 0.068 -1.922 –
Cavallo et al. 2024 267.491 -33.361 0.642 – – –
Hunt & Reffert 2023 267.466 -33.335 0.639 0.068 -1.922 –
He et al. 2023 267.466 -33.363 0.654 0.02 -2.017 –

💡 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 – – – – – 261* – –
Cavallo et al. 2024 1.06 3.10 – 25 -0.720 – – –
Hunt & Reffert 2023 1.42 2.34 1.78 106 – – – –
He et al. 2023 1.48 2.25 – 200 – – – –

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

Visualization

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