CWNU 183

Click to load Aladin Lite
0.25 UTI
0.0
CN
0.25
Cdens
0.5
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 7.5 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.25 Loose
  • CC3 0.5 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

â„šī¸
CWNU 183 is a sparse, loose object of intermediate C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, very young cluster, but with a large variance across recent sources for the age parameter (see Parameters). It is poorly studied in the literature.
Relatively close Moderate extinction Near-solar metallicity Very young

Cavallo et al. (2024)
Gold sample.

Data

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 273.11 -21.115 0.561 0.353 -1.682 -4.247
Hunt & Reffert 2024 273.088 -21.143 0.568 0.417 -1.729 –
Cavallo et al. 2024 273.082 -21.148 0.57 – – –
Hunt & Reffert 2023 273.088 -21.143 0.568 0.417 -1.729 –
He et al. 2022 273.099 -21.11 0.59 0.21 -1.47 -4.4

💡 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 – – – – – 217* – –
Cavallo et al. 2024 1.79 2.94 – 4 -0.840 – – –
Hunt & Reffert 2023 1.67 2.48 1.45 33 – – – –
He et al. 2022 2.34 3.66 – 8 0.169 – – –

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

Visualization

â„šī¸