CWNU 2490

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0.48 UTI
0.26
CN
1.0
Cdens
0.62
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 1.3 [arcmin]
  • CN 0.26 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.62 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 2490 is a poorly populated, very dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.
Relatively close 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 – 58.989 55.336 0.323 -0.446 -0.727 –
Hunt & Reffert 2024 58.992 55.335 0.296 -0.442 -0.717 –
Cavallo et al. 2024 59.003 55.356 0.309 – – –
Hunt & Reffert 2023 58.992 55.335 0.296 -0.442 -0.717 –
He et al. 2023 58.991 55.337 0.321 -0.449 -0.73 –

💡 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 – – – – – 219* – –
Cavallo et al. 2024 2.90 2.79 – 48 -0.400 – – –
Hunt & Reffert 2023 2.98 2.47 1.00 110 – – – –
He et al. 2023 2.95 2.65 – 112 – – – –

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

Visualization

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