CWNU 2678

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) 1.8 [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 2678 is a sparse, very dense object of low C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It was recently reported in the literature.
Relatively close Moderate extinction Near-solar metallicity 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 – 149.942 -58.127 0.354 -6.83 4.797 –
Hunt & Reffert 2024 149.937 -58.124 0.347 -6.806 4.775 –
Cavallo et al. 2024 149.953 -58.127 0.346 – – –
Hunt & Reffert 2023 149.937 -58.124 0.347 -6.806 4.775 –
He et al. 2023 149.947 -58.121 0.363 -6.811 4.812 –

💡 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 – – – – – 133* – –
Cavallo et al. 2024 2.58 1.72 – 32 0.030 – – –
Hunt & Reffert 2023 2.70 1.62 0.59 60 – – – –
He et al. 2023 2.45 1.85 – 50 – – – –

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

Visualization

â„šī¸