CWNU 1303

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0.54 UTI
0.47
CN
1.0
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 4.1 [arcmin]
  • CN 0.47 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 1303 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 near-solar metallicity, very young cluster (see Parameters). It was recently reported in the literature.
Relatively close High extinction Near-solar metallicity Very young

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 – 261.212 -37.765 0.426 -0.108 -1.2 41.225
Hunt & Reffert 2024 261.237 -37.741 0.429 -0.098 -1.215 69.038
Cavallo et al. 2024 261.192 -37.768 0.429 – – –
Hunt & Reffert 2023 261.237 -37.741 0.429 -0.098 -1.215 69.038
He et al. 2023 261.21 -37.759 0.425 -0.103 -1.2 –

💡 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 – – – – – 747* – –
Cavallo et al. 2024 2.21 3.23 – 11 0.420 – – –
Hunt & Reffert 2023 2.22 3.20 2.49 7 – – – –
He et al. 2023 2.34 3.65 – 5 – – – –

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

Visualization

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