HSC 2003

Click to load Aladin Lite
0.17 UTI
0.25
CN
0.25
Cdens
0.38
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 3.9 [arcmin]
  • CN 0.25 Poorly populated
  • Cdens 0.25 Loose
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 2003 is a poorly populated, loose 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, intermediate-age cluster (see Parameters). It was recently reported in the literature.

âš ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Distant Moderate extinction Near-solar metallicity Intermediate age

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 – 119.147 -32.508 0.252 -2.934 3.72 –
Hunt & Reffert 2024 119.126 -32.539 0.252 -2.91 3.701 –
Cavallo et al. 2024 119.153 -32.502 0.252 – – –
Hunt & Reffert 2023 119.126 -32.539 0.252 -2.91 3.701 –

💡 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 – – – – – 190* – –
Cavallo et al. 2024 3.52 1.73 – 437 -0.060 – – –
Hunt & Reffert 2023 3.46 1.61 2.06 177 – – – –

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

Visualization

â„šī¸