CWNU 2847

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0.44 UTI
0.33
CN
0.62
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 5.0 [arcmin]
  • CN 0.33 Poorly populated
  • Cdens 0.62 Moderately dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 2847 is a poorly populated, moderately 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 near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.
Relatively close High 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 – 280.4 -4.209 0.444 -0.825 -0.617 -26.891
Hunt & Reffert 2024 280.391 -4.178 0.45 -0.864 -0.608 -25.942
Cavallo et al. 2024 280.401 -4.228 0.45 – – –
Hunt & Reffert 2023 280.391 -4.178 0.45 -0.864 -0.608 -25.942
He et al. 2023 280.43 -4.221 0.449 -0.823 -0.595 -27.18

💡 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 – – – – – 464* – –
Cavallo et al. 2024 1.67 4.33 – 288 0.120 – – –
Hunt & Reffert 2023 2.10 4.09 1.79 189 – – – –
He et al. 2023 2.04 3.80 – 562 – – – –

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

Visualization

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