CWNU 1275

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0.52 UTI
0.58
CN
1.0
Cdens
0.5
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 2.5 [arcmin]
  • CN 0.58 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 0.5 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 1275 is a moderately populated, very 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 – 227.183 -59.646 0.338 -3.752 -2.855 -28.77
Hunt & Reffert 2024 227.216 -59.645 0.335 -3.766 -2.907 -21.226
Cavallo et al. 2024 227.21 -59.642 0.337 – – –
Hunt & Reffert 2023 227.216 -59.645 0.335 -3.766 -2.907 -21.226
He et al. 2023 227.213 -59.645 0.347 -3.757 -2.856 –

💡 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 – – – – – 1434* – –
Cavallo et al. 2024 3.75 4.92 – 40 0.370 – – –
Hunt & Reffert 2023 2.66 4.38 2.81 157 – – – –
He et al. 2023 2.69 5.60 – 4 – – – –

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

Visualization

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