CWNU 2825

Click to load Aladin Lite
0.55 UTI
0.48
CN
1.0
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 2.9 [arcmin]
  • CN 0.48 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

â„šī¸
CWNU 2825 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by very high extinction. It is catalogued as a massive, near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.
Relatively close Very high extinction Massive Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Silver sample.

Data

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 272.086 -21.038 0.332 0.509 -1.161 18.622
Hunt & Reffert 2024 272.096 -21.062 0.332 0.519 -1.147 29.576
Cavallo et al. 2024 272.089 -21.043 0.33 – – –
Hunt & Reffert 2023 272.096 -21.062 0.332 0.519 -1.147 29.576
He et al. 2023 272.079 -21.041 0.348 0.507 -1.154 20.26

💡 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 – – – – – 1614* – –
Cavallo et al. 2024 2.61 5.08 – 195 -0.010 – – –
Hunt & Reffert 2023 2.68 4.98 2.92 240 – – – –
He et al. 2023 2.40 5.20 – 501 – – – –

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

Visualization

â„šī¸