CWNU 1506

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0.30 UTI
0.25
CN
0.25
Cdens
0.5
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 4.9 [arcmin]
  • CN 0.25 Poorly populated
  • Cdens 0.25 Loose
  • CC3 0.5 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

CWNU 1506 is a poorly populated, loose object of intermediate C3 quality. Its parallax locates it at a moderate distance, below the mid-plane. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It was recently reported in the literature.

Data

Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 356.204 59.674 0.321 -2.721 -1.879
Hunt & Reffert 2024 356.136 59.673 0.326 -2.71 -1.88
Cavallo et al. 2024 356.187 59.663 0.326
Hunt & Reffert 2023 356.136 59.673 0.326 -2.71 -1.88
He et al. 2023 356.25 59.648 0.321 -2.721 -1.911

💡 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 280*
Cavallo et al. 2024 2.94 2.51 23 0.200
Hunt & Reffert 2023 2.75 2.77 1.73 12
He et al. 2023 2.95 3.05 6

💡 Note: The parameters are sometimes transformed from their original values to match the format of the columns shown here, see FAQ. The columns DAv, Bfr, BSS correspond to differential extinction, binary fraction, and blue stragglers, respectively. BSS values can be listed as fractions or integers.
(*): indicates that this parameter is assigned more than one value in the corresponding reference.

Visualization

Galactocentric position diagram

💡 Note: How are the galactocentric plots generated? See FAQ.