CWNU 1677

Click to load Aladin Lite
0.50 UTI
0.32
CN
0.92
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 3.1 [arcmin]
  • CN 0.32 Poorly populated
  • Cdens 0.92 Very dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

CWNU 1677 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane. It is catalogued as a near-solar metallicity, intermediate-age 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 210.654 -59.414 0.343 -4.841 -2.881 -35.973
Hunt & Reffert 2024 210.687 -59.423 0.331 -4.851 -2.874 -35.844
Cavallo et al. 2024 210.533 -59.396 0.332
Hunt & Reffert 2023 210.687 -59.423 0.331 -4.851 -2.874 -35.844
He et al. 2023 210.615 -59.411 0.346 -4.83 -2.889 -36.39

💡 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 445*
Cavallo et al. 2024 2.40 2.53 437 0.280
Hunt & Reffert 2023 2.70 2.84 2.17 159
He et al. 2023 2.63 3.05 355

💡 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.