CWNU 1376

Click to load Aladin Lite
0.46 UTI
0.29
CN
1.0
Cdens
0.5
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 1.2 [arcmin]
  • CN 0.29 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.5 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

â„šī¸
CWNU 1376 is a poorly populated, very dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It was recently reported in the literature.
Relatively close Low 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 – 331.321 52.388 0.368 -3.511 -2.072 –
Hunt & Reffert 2024 331.323 52.394 0.354 -3.521 -2.084 –
Cavallo et al. 2024 331.33 52.399 0.361 – – –
Hunt & Reffert 2023 331.323 52.394 0.354 -3.521 -2.084 –
He et al. 2023 331.313 52.399 0.374 -3.529 -2.065 –

💡 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 – – – – – 204* – –
Cavallo et al. 2024 2.58 0.97 – 71 0.030 – – –
Hunt & Reffert 2023 2.56 0.79 0.90 121 – – – –
He et al. 2023 2.45 1.05 – 40 – – – –

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

Visualization

â„šī¸