CWNU 1818

Click to load Aladin Lite
0.25 UTI
0.0
CN
0.23
Cdens
0.5
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 9.0 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.23 Very loose
  • CC3 0.5 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

â„šī¸
CWNU 1818 is a sparse, very 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, intermediate-age cluster (see Parameters). It was recently reported in the literature.
Relatively close Moderate extinction Near-solar metallicity Intermediate age

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 – 316.227 47.717 0.573 -2.697 -3.582 –
Hunt & Reffert 2024 316.268 47.687 0.575 -2.683 -3.607 –
Cavallo et al. 2024 316.253 47.717 0.574 – – –
Hunt & Reffert 2023 316.268 47.687 0.575 -2.683 -3.607 –
He et al. 2023 316.33 47.724 0.576 -2.703 -3.564 –

💡 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 – – – – – 126* – –
Cavallo et al. 2024 1.77 2.05 – 191 -0.230 – – –
Hunt & Reffert 2023 1.70 2.04 0.72 272 – – – –
He et al. 2023 1.70 2.15 – 28 – – – –

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

Visualization

â„šī¸