HSC 1083

Click to load Aladin Lite
0.44 UTI
0.37
CN
0.59
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 2.7 [arcmin]
  • CN 0.37 Poorly populated
  • Cdens 0.59 Moderately dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 1083 is a poorly populated, moderately dense object of high C3 quality. Its parallax locates it at a moderate distance, well above the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, old cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It was recently reported in the literature.

Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.

Distant High extinction Near-solar metallicity Old

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 – 40.891 67.593 0.223 -0.338 -0.475 -22.344
Hu & Soubiran 2025 40.948 67.61 – – – –
Hunt & Reffert 2024 40.882 67.627 0.215 -0.345 -0.463 -16.132
Cavallo et al. 2024 40.948 67.61 0.219 – – –
Hunt & Reffert 2023 40.882 67.627 0.215 -0.345 -0.463 -16.132

💡 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
Hu & Soubiran 2025 – – – – 0.190* – – –
Hunt & Reffert 2024 – – – – – 572* – –
Cavallo et al. 2024 3.53 3.64 – 1259 -0.390 – – –
Hunt & Reffert 2023 3.92 3.47 1.52 1194 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3356 81.1 40.9 67.59 0.22 -0.33 -0.48 -22.34 0.01

💡 Note: The % column shows the percentage of members that HSC 1083 shares with each listed object.

Visualization

â„šī¸