CWNU 2310

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0.53 UTI
0.39
CN
1.0
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 1.9 [arcmin]
  • CN 0.39 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 2310 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a massive, metal-poor, very young cluster (see Parameters). It was recently reported in the literature.
Distant High extinction Massive Metal-poor Very young

Cavallo et al. (2024)
Silver sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 280.411 -6.464 0.247 -1.197 -3.66 44.774
Hunt & Reffert 2024 280.414 -6.466 0.24 -1.193 -3.653 49.253
Cavallo et al. 2024 280.412 -6.454 0.241 – – –
Hunt & Reffert 2023 280.414 -6.466 0.24 -1.193 -3.653 49.253
He et al. 2023 280.411 -6.467 0.257 -1.207 -3.658 53.1

💡 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 – – – – – 1138* – –
Cavallo et al. 2024 2.50 3.67 – 3 -0.940 – – –
Hunt & Reffert 2023 3.75 3.35 3.03 12 – – – –
He et al. 2023 4.47 3.85 – 4 – – – –

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

Visualization

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