CWNU 1615

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0.57 UTI
0.42
CN
0.91
Cdens
1.0
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 7.0 [arcmin]
  • CN 0.42 Poorly populated
  • Cdens 0.91 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 1615 is a poorly populated, very dense object of very high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a metal-poor, young cluster (see Parameters). It was recently reported in the literature.
Relatively close Moderate extinction Metal-poor 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 – 271.131 -26.065 0.671 1.451 0.442 -22.6
Hunt & Reffert 2024 271.133 -26.028 0.651 1.381 0.501 -11.884
Cavallo et al. 2024 271.171 -26.069 0.651 – – –
Hunt & Reffert 2023 271.133 -26.028 0.651 1.381 0.501 -11.884
He et al. 2023 271.114 -26.064 0.674 1.463 0.436 –

💡 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 – – – – – 360* – –
Cavallo et al. 2024 1.09 2.54 – 26 -0.770 – – –
Hunt & Reffert 2023 1.46 1.59 2.44 61 – – – –
He et al. 2023 1.41 2.20 – 32 – – – –

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

Visualization

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