CWNU 2277

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0.48 UTI
0.46
CN
0.84
Cdens
0.62
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 3.7 [arcmin]
  • CN 0.46 Poorly populated
  • Cdens 0.84 Dense
  • CC3 0.62 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 2277 is a poorly populated, dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a massive, near-solar metallicity, young cluster (see Parameters). It was recently reported in the literature.
Relatively close High extinction Massive Near-solar metallicity 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 – 279.918 -8.419 0.325 -0.275 -2.97 52.334
Hunt & Reffert 2024 279.901 -8.423 0.31 -0.271 -2.958 101.355
Cavallo et al. 2024 279.903 -8.431 0.309 – – –
Hunt & Reffert 2023 279.901 -8.423 0.31 -0.271 -2.958 101.355
He et al. 2023 279.907 -8.423 0.331 -0.27 -2.989 38.16

💡 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 – – – – – 1317* – –
Cavallo et al. 2024 2.41 4.13 – 60 -0.280 – – –
Hunt & Reffert 2023 2.89 4.04 2.68 74 – – – –
He et al. 2023 2.57 3.70 – 447 – – – –

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

Visualization

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