CWNU 1807

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0.31 UTI
0.0
CN
0.8
Cdens
0.25
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 3.1 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.8 Dense
  • CC3 0.25 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

CWNU 1807 is a sparse, dense object of low C3 quality. Its parallax locates it at a moderate distance, near the mid-plane. It is catalogued as a metal-rich, 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 77.236 40.501 0.368 0.163 -0.821 -18.564
Hunt & Reffert 2024 77.279 40.505 0.371 0.144 -0.809 -28.88
Cavallo et al. 2024 77.248 40.536 0.366
Hunt & Reffert 2023 77.279 40.505 0.371 0.144 -0.809 -28.88
He et al. 2023 77.244 40.513 0.378 0.172 -0.826 -23.82

💡 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 145*
Cavallo et al. 2024 2.54 0.99 490 0.650
Hunt & Reffert 2023 2.55 1.15 1.20 417
He et al. 2023 2.40 1.40 631

💡 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.