CWNU 2298

Click to load Aladin Lite
0.38 UTI
0.0
CN
1.0
Cdens
0.38
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 2.2 [arcmin]
  • CN 0.0 Sparse
  • Cdens 1.0 Very dense
  • CC3 0.38 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

â„šī¸
CWNU 2298 is a sparse, very dense object of low C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by high extinction. It is catalogued as a metal-rich, young cluster (see Parameters). It was recently reported in the literature.
Relatively close High extinction Metal-rich Young

Cavallo et al. (2024)
Bronze sample.

Data

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 316.864 50.123 0.509 -3.16 -4.177 –
Hunt & Reffert 2024 316.867 50.128 0.491 -3.127 -4.17 –
Cavallo et al. 2024 316.851 50.102 0.5 – – –
Hunt & Reffert 2023 316.867 50.128 0.491 -3.127 -4.17 –
He et al. 2023 316.865 50.131 0.509 -3.16 -4.177 –

💡 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 – – – – – 257* – –
Cavallo et al. 2024 2.70 3.31 – 50 0.960 – – –
Hunt & Reffert 2023 1.84 3.96 2.33 49 – – – –
He et al. 2023 2.04 4.50 – 13 – – – –

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

Visualization

â„šī¸