CWNU 2758

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0.62 UTI
0.6
CN
1.0
Cdens
1.0
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 2.7 [arcmin]
  • CN 0.6 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 2758 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by high extinction. It is catalogued as a massive, near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.
Distant High extinction Massive Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Bronze sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 295.421 26.147 0.223 -2.517 -4.751 -2.445
Hunt & Reffert 2024 295.422 26.15 0.202 -2.538 -4.791 20.562
Cavallo et al. 2024 295.39 26.13 0.203 – – –
Hunt & Reffert 2023 295.422 26.15 0.202 -2.538 -4.791 20.562
He et al. 2023 295.399 26.138 0.234 -2.529 -4.758 -4.69

💡 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 – – – – – 2444* – –
Cavallo et al. 2024 5.04 3.92 – 51 0.190 – – –
Hunt & Reffert 2023 4.44 3.98 2.97 153 – – – –
He et al. 2023 3.72 3.70 – 398 – – – –

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

Visualization

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