CWNU 98

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0.38 UTI
0.3
CN
0.61
Cdens
0.5
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 7.2 [arcmin]
  • CN 0.3 Poorly populated
  • Cdens 0.61 Moderately dense
  • CC3 0.5 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 98 is a poorly populated, moderately dense object of intermediate C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is poorly studied in the literature.
Relatively close Moderate extinction Near-solar metallicity Young

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 – 275.961 -9.901 0.667 0.2 -3.497 5.291
Hunt & Reffert 2024 275.963 -9.888 0.666 0.191 -3.502 5.284
Cavallo et al. 2024 275.947 -9.893 0.665 – – –
Hunt & Reffert 2023 275.963 -9.888 0.666 0.191 -3.502 5.284
He et al. 2022 275.977 -9.878 0.68 0.25 -3.48 –

💡 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 – – – – – 152* – –
Cavallo et al. 2024 1.26 2.88 – 178 -0.700 – – –
Hunt & Reffert 2023 1.43 1.91 0.81 90 – – – –
He et al. 2022 1.86 2.40 – 32 0.968 – – –

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

Visualization

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