CWNU 2350

Click to load Aladin Lite
0.58 UTI
0.68
CN
0.97
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 2.7 [arcmin]
  • CN 0.68 Moderately populated
  • Cdens 0.97 Very dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

â„šī¸
CWNU 2350 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a large distance, above the mid-plane, affected by high extinction. It is catalogued as a massive, near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.
Distant High extinction Massive Near-solar metallicity Intermediate age

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 – 182.61 -62.051 0.187 -7.795 1.099 -15.194
Hunt & Reffert 2024 182.591 -62.041 0.192 -7.786 1.092 -3.844
Cavallo et al. 2024 182.613 -62.046 0.195 – – –
Hunt & Reffert 2023 182.591 -62.041 0.192 -7.786 1.092 -3.844
He et al. 2023 182.618 -62.052 0.212 -7.798 1.112 -15.19

💡 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 – – – – – 2246* – –
Cavallo et al. 2024 5.30 3.91 – 234 -0.130 – – –
Hunt & Reffert 2023 4.52 3.80 2.51 468 – – – –
He et al. 2023 4.17 3.45 – 1000 – – – –

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

Visualization

â„šī¸